Equilateral non-Gaussianity from heavy fields
High Energy Physics - Theory
2015-06-16 v1 Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
Abstract
The effect of self-interactions of heavy scalar fields during inflation on the primordial non-Gaussianity is studied. We take a specific constant-turn quasi-single field inflation as an example. We derive an effective theory with emphasis on non-linear self-interactions of heavy fields and calculate the corresponding non-Gaussianity, which is of equilateral type and can be as relevant as those computed previously in the literature. We also derive the non-Gaussianity by directly using the in-in formalism, and verify the equivalence of these two approaches.
Cite
@article{arxiv.1306.3691,
title = {Equilateral non-Gaussianity from heavy fields},
author = {Jinn-Ouk Gong and Shi Pi and Misao Sasaki},
journal= {arXiv preprint arXiv:1306.3691},
year = {2015}
}
Comments
17 pages, 1 figure