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Abstract We study reheating of inflationary models with general non-minimal coupling K (ϕ) R with K (ϕ) ∼ √( V (ϕ)) where R is the Ricci scalar and R is the inflaton potential. In particular, when we take the monomial potential K (ϕ) ∝ ϕ m with m ∈ℤ + , we provide general analytic expressions for cosmological observables. We consider a wide range of non-minimal coupling ξ∈[0,∞) in metric and Palatini formalisms and derive the predictions for cosmological observables and the reheating temperature taking a general equation of state parameter w reh .
Cheong et al. (Tue,) studied this question.
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