Abstract

Conventional wisdom says that a chaotic inflation model with a power-law potential is ruled out by the recent Planck-BICEP/Keck results. We find, however, that the model can be assisted by a non-minimally coupled scalar field and still provides a successful inflation. Considering a power-law chaotic inflation model of the type V∼φnV\sim φ^n with n={2,4/3,1,2/3,1/3}n=\{2, 4/3, 1, 2/3, 1/3\}, we show that n=1/3n=1/3 (n={2/3,1/3}n=\{2/3, 1/3\}) may be revived with the help of the quadratic (quartic) non-minimal coupling of the assistant field to gravity.

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