Abstract:
This study proposes a novel parametrization approach for the dimensionless Hubble parameter i.e. 𝐸2
(𝑧) =
𝐴(𝑧) + 𝛽(1 + 𝛾𝐵(𝑧)) in the context of scalar field dark energy models. The parametrization is characterized by
two functions, 𝐴(𝑧) and 𝐵(𝑧), carefully chosen to capture the behavior of the Hubble parameter at different
redshifts. We explore the evolution of cosmological parameters, including the deceleration parameter, density
parameter, and equation of state parameter. Observational data from Cosmic Chronometers (CC), Baryonic
Acoustic Oscillations (BAO), and the Pantheon+ datasets are analyzed using MCMC methodology to determine
model parameters. The results are compared with the standard 𝛬CDM model using the Planck observations.
Our approach provides a model-independent exploration of dark energy, contributing to a comprehensive
understanding of late-time cosmic acceleration.
