English

Non-Gaussianity in the warm k-inflation

General Relativity and Quantum Cosmology 2023-06-28 v3 Cosmology and Nongalactic Astrophysics

Abstract

This paper presents and investigates non-Gaussian perturbations for the warm k-inflation model that is driven by pure kinetic energy. The two complementary components of the overall non-Gaussianity are the three-point and four-point correlations. The intrinsic non-Gaussian component, denoted as the nonlinear parameter f_{NL}^{int}, is rooted in the three-point correlation for the inflaton field. Meanwhile, the \delta N part non-Gaussianity, denoted as f_{NL}^{\delta N}, is the contribution attributed to the four-point correlation function of the inflaton field. In this paper, the above two components in warm k-inflation are individually computed and analyzed. Then, comparisons and discussions between them are conducted, and the non-Gaussian theoretical results are compared with experimental observations to determine the range of model parameters within the allowable range of observation.

Keywords

Cite

@article{arxiv.2303.05260,
  title  = {Non-Gaussianity in the warm k-inflation},
  author = {Chao-Qun Shen and Xiao-Min Zhang and Zhi-Peng Peng and He Liu and Xi-Bin Li and Peng-Cheng Chu},
  journal= {arXiv preprint arXiv:2303.05260},
  year   = {2023}
}