Curvaton in large field inflation

Abstract

We comprehensively explore the quadratic curvaton models in the chaotic inflation. In the light of the BICEP2 result r ≈ 0.2, all model parameters and relevant observables are computed. It is found the curvaton field value is constrained into a narrow range, σ* = O(10-2-10-1) and the running of the spectral index is ns' -10-3. We show that if the curvaton is added, the models are heavily degenerated on the ns - r plane. However, introducing a new plane, the degeneracy can be resolved. To distinguish the curvaton models, precise measurements of not only r but also ns' and the tensor tilt nT are required.

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