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Curvaton in large field inflation

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arxiv 1404.0951 v2 pith:MT6AEV5I submitted 2014-04-03 astro-ph.CO gr-qchep-ph

Curvaton in large field inflation

classification astro-ph.CO gr-qchep-ph
keywords curvatonmodelsfieldinflationplaneaddedapproxbicep2
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We comprehensively explore the quadratic curvaton models in the chaotic inflation. In the light of the BICEP2 result $r \approx 0.2$, all model parameters and relevant observables are computed. It is found the curvaton field value is constrained into a narrow range, $\sigma_* = \mathcal{O}(10^{-2}$-$10^{-1})$ and the running of the spectral index is $n_s' \gtrsim -10^{-3}$. We show that if the curvaton is added, the models are heavily degenerated on the $n_s$ - $r$ plane. However, introducing a new plane, the degeneracy can be resolved. To distinguish the curvaton models, precise measurements of not only $r$ but also $n_s'$ and the tensor tilt $n_T$ are required.

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