Composite Inflation confronts BICEP2 and PLANCK

TL;DR

This paper investigates how different composite inflation models align with recent Planck and BICEP2 observational data, highlighting which models are compatible with these constraints and identifying parameter ranges that fit the observations.

Contribution

It provides a comparative analysis of multiple composite inflation models against the latest cosmological data, revealing their viability and parameter constraints.

Findings

MCI model fits Planck data but conflicts with BICEP2 in large non-minimal coupling.

GI model satisfies Planck data and can match BICEP2 with fewer e-foldings.

Super Yang-Mills model aligns with Planck and can produce BICEP2-compatible tensor-to-scalar ratios.

Abstract

We examine observational constraints on single-field inflation in which the inflaton is a composite field stemming from a four-dimensional strongly interacting field theory. We confront the predictions with the Planck and very recent BICEP2 data. In the large non-minimal coupling regions, we discover for MCI model that the predictions lie well inside the joint $68\%$ CL for the Planck data, but is in tension with the recent BICEP2 observations. In the case of the GI model, the predictions satisfy the Planck results. However, this model can produce a large tensor-to-scalar ratio consistent with the recent BICEP2 observations if the number of e-foldings is slightly smaller than the range commonly used. For a super Yang-Mills paradigm, we discover that the predictions satisfy the Planck data, and surprisingly a large tensor-to-scalar ratio consistent with the BICEP2 results can also be produced for an acceptable range of the number of e-foldings and of the confining scale. In the small non-minimal coupling regions, all of the models can satisfy the BICEP2 results. However, the predictions of GI and SgbI models cannot satisfy the observational bound on the amplitude of the curvature perturbation launched by Planck, and the techni-inflaton self-coupling in the MCI model is constrained to be extremely small.