Nonminimal Coleman--Weinberg Inflation with an term
arXiv:1810.12884 · doi:10.1088/1475-7516/2019/02/006
Abstract
We extend the Coleman--Weinberg inflationary model where a scalar field is non-minimally coupled to gravity with the addition of the term. We express the theory in terms of two scalar fields and going to the Einstein frame we employ the Gildener--Weinberg formalism, compute the one-loop effective potential and essentially reduce the problem to the case of single-field inflation. It turns out that there is only one free parameter, namely, the mixing angle between the scalars. For a wide range of this angle, we compute the inflationary observables which are in agreement with the latest experimental bounds. The effect of the term is that it lowers the value of the tensor-to-scalar ratio .
arXiv commenttypos fixed, equation (3.16) and discussion around it added, updated references
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