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