pith. sign in

arxiv: 1404.0951 · v2 · pith:MT6AEV5Inew · submitted 2014-04-03 · 🌌 astro-ph.CO · gr-qc· hep-ph

Curvaton in large field inflation

classification 🌌 astro-ph.CO gr-qchep-ph
keywords curvatonmodelsfieldinflationplaneaddedapproxbicep2
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.