English

Perturbation, Non-Gaussianity and Reheating in a GB-$\alpha$-Attractor Model

Cosmology and Nongalactic Astrophysics 2017-08-02 v2 General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

Motivated by α\alpha-attractor models, in this paper we consider a Gauss-Bonnet inflation with E-model type of potential. We consider the Gauss-Bonnet coupling function to be the same as the E-model potential. In the small α\alpha limit we obtain an attractor at r=0r=0 as expected, and in the large α\alpha limit we recover the Gauss-Bonnet model with potential and coupling function of the form ϕ2n\phi^{2n}. We study perturbations and non-Gaussianity in this setup and we find some constraints on the model's parameters in comparison with PLANCK datasets. We study also the reheating epoch after inflation in this setup. For this purpose, we seek the number of e-folds and temperature during reheating epoch. These quantities depend on the model's parameter and the effective equation of state of the dominating energy density in the reheating era. We find some observational constraints on these parameters.

Keywords

Cite

@article{arxiv.1705.02617,
  title  = {Perturbation, Non-Gaussianity and Reheating in a GB-$\alpha$-Attractor Model},
  author = {Kourosh Nozari and Narges Rashidi},
  journal= {arXiv preprint arXiv:1705.02617},
  year   = {2017}
}

Comments

12 pages, 4 figures, Revised version, to appear in PRD