Curvaton reheating in logamediate inflationary model

TL;DR

This paper explores how the curvaton field can end inflation and reheat the universe within a logamediate inflationary model, providing constraints on model parameters and reheating temperature.

Contribution

It introduces the curvaton mechanism into the logamediate inflationary model and determines the reheating temperature along with parameter constraints.

Findings

Reheating temperature is derived for the model.

Parameter space constraints are established.

The curvaton field effectively ends inflation in this scenario.

Abstract

In a logamediate inflationary universe model we introduce the curvaton field in order to bring this inflationary model to an end. In this approach we determine the reheating temperature. We also outline some interesting constraints on the parameters that describe our models. Thus, we give the parameter space in this scenario.