English

Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation

Cosmology and Nongalactic Astrophysics 2010-04-06 v3 High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We study the slow-roll inflation models, where the inflaton slow-rolls along a trajectory whose orthogonal directions are lifted by potentials with masses of order the Hubble parameter. In these models large non-Gaussianities can be generated through the transformation from the isocurvature modes to the curvature mode, once the inflaton trajectory turns. We find large bispectra with one-parameter family of novel shapes, interpolating between the equilateral and local shape. According to the in-in formalism, the shapes of these non-Gaussianities are different from a simple projection from the isocurvature non-Gaussian correlation functions.

Keywords

Cite

@article{arxiv.0909.0496,
  title  = {Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation},
  author = {Xingang Chen and Yi Wang},
  journal= {arXiv preprint arXiv:0909.0496},
  year   = {2010}
}

Comments

5 pages, v3, minor revision, PRD version