English

Anomalous Dimensions and Non-Gaussianity

High Energy Physics - Theory 2015-06-12 v1 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

Abstract

We analyze the signatures of inflationary models that are coupled to strongly interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the bispectrum, we find a simple scaling behavior determined by operator dimensions, which are constrained by the appropriate unitarity bounds. Specifically, we analyze two simple and calculable classes of examples: conformal field theories (CFTs), and large-N CFTs deformed by relevant time-dependent double-trace operators. Together these two classes of examples exhibit a wide range of scalings and shapes of the bispectrum, including nearly equilateral, orthogonal and local non-Gaussianity in different regimes. Along the way, we compare and contrast the shape and amplitude with previous results on weakly coupled fields coupled to inflation. This signature provides a precision test for strongly coupled sectors coupled to inflation via irrelevant operators suppressed by a high mass scale up to 1000 times the inflationary Hubble scale.

Keywords

Cite

@article{arxiv.1301.2630,
  title  = {Anomalous Dimensions and Non-Gaussianity},
  author = {Daniel Green and Matthew Lewandowski and Leonardo Senatore and Eva Silverstein and Matias Zaldarriaga},
  journal= {arXiv preprint arXiv:1301.2630},
  year   = {2015}
}

Comments

40 pages, 10 figures

R2 v1 2026-06-21T23:08:10.369Z