Reconstructions of the dark-energy equation of state and the inflationary potential

TL;DR

This paper develops a mathematical framework to reconstruct the dark-energy equation of state and inflationary potential from observed spectral indices, exploring different functional forms and solution mappings.

Contribution

It introduces a method to derive explicit cosmological solutions from spectral index data using constraints and mappings, advancing understanding of inflation and dark energy.

Findings

Derived explicit forms for the scale factor and potential

Established mappings to generate new cosmological solutions

Analyzed cases with different functional forms of h(r)

Abstract

We use a mathematical approach based on the constraints systems in order to reconstruct the equation of state and the inflationary potential for the inflaton field from the observed spectral indices for the density perturbations $n_{s}$ and the tensor to scalar ratio $r$. From the astronomical data, we can observe that the measured values of these two indices lie on a two-dimensional surface. We express these indices in terms of the Hubble slow-roll parameters and we assume that $n_{s}-1=h\left( r\right) $. For the function $h\left( r\right) $, we consider three cases, where $h\left( r\right) $ is constant, linear and quadratic, respectively. From this, we derive second-order equations whose solutions provide us with the explicit forms for the expansion scale-factor, the scalar-field potential, and the effective equation of state for the scalar field. Finally, we show that for there exist mappings which transform one cosmological solution to another and allow new solutions to be generated from existing ones.