Inflationary Dynamics in Einstein-Gauss-Bonnet Gravity Using New Slow-Roll Approximations considering Generalised Reheating

TL;DR

This paper explores inflationary dynamics within Einstein-Gauss-Bonnet gravity using new slow-roll approximations and generalized reheating, demonstrating compatibility with observations and avoiding late-stage thermal inflation.

Contribution

It introduces a novel application of new slow-roll approximations to the Power Law Plateau inflation model in EGB gravity, incorporating generalized reheating effects.

Findings

Model aligns with Planck observations

Avoids late-stage thermal inflation

Provides a new framework for inflationary analysis in EGB gravity

Abstract

The Cosmic Microwave Background (CMB) observations results reported by {\it Planck} satellite suggest a plateau characteristic in the flat potential of the inflaton field is favored to drive the Universe's early acceleration. On that note, Power Law Plateau (PLP) potential has gained a lot of attention. In this study, we demonstrate that implementing this inflationary model in an Einstein-Gauss-Bonnet(EGB) gravity background makes the model compatible with observations while avoiding late-stage thermal inflation which is otherwise unavoidable in a standard scenario. More importantly, we have taken the PLP model as a case study to check the new slow-roll approximations method proposed in \cite{Pozdeeva:2024ihc}. Then we take one step further to check the consequence of generalized reheating in this scenario. Thus opening a new promising window to study inflationary dynamics in EGB gravity.