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arXiv:1404.0951·v2·Cosmology and Nongalactic Astrophysics

Curvaton in large field inflation

Tomohiro Fujita🇯🇵 · Masahiro Kawasaki🇯🇵 · Shuichiro Yokoyama🇯🇵

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Abstract

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

Comments: 16pages, 12figures, ver2: typo corrected, figs. 5-9 and 11 are revised

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