A generalized equation of state for dark energy

TL;DR

This paper introduces a new generalized parameterization for dark energy's equation of state, unifying existing models and expanding the range of possible cosmological solutions, with implications for observational constraints.

Contribution

A novel generalized equation of state parameterization for dark energy that encompasses known models and allows for a broader set of cosmological solutions.

Findings

Recovers known EoS models at specific parameter limits

Proposes a wider range of cosmological solutions

Discusses potential observational constraints

Abstract

A generalized parameterization $w_\beta(z)$ for the dark energy equation of state (EoS) is proposed and some of its cosmological consequences are investigated. We show that in the limit of the characteristic dimensionless parameter $\beta \to +1, 0$ and -1 some well-known EoS parameterizations are fully recovered whereas for other values of $\beta$ the proposed parameterization admits a wider and new range of cosmological solutions. We also discuss possible constraints on the $w_\beta(z)$ parameters from current observational data.