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- W2166022723 abstract "We derive the consistency relations for a chaotic inflation model with a non-minimal coupling to gravity. For a quadratic potential in the limit of a small non-minimal coupling parameter |$xi$| and for a quartic potential without assuming small |$xi$|, we give the consistency relations among the 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 |$rlt 0.1$|, then |$xi$| is constrained to |$xi lt 0$| and |$alpha$| is predicted to be |$alpha simeq {-}8 times 10^{-4}$| for a quartic potential. For a general monomial potential, |$alpha$| is constrained in the range |$-2.7times 10^{-3} lt alpha lt -6 times 10^{-4}$| as long as |$|xi |leq 10^{-3}$| if |$rlt 0.1$|." @default.
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- W2166022723 date "2015-02-23" @default.
- W2166022723 modified "2023-09-23" @default.
- W2166022723 title "Consistency relations for large-field inflation: Non-minimal coupling" @default.
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- W2166022723 doi "https://doi.org/10.1093/ptep/ptv007" @default.
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