Quintessence scalar field model in Weyl-type $f(Q,T)$ Gravity with $w_D-w'_D$ analysis
Vinod Kumar Bhardwaj, Priyanka Garg

TL;DR
This paper investigates a quintessence cosmological model within Weyl-type $f(Q,T)$ gravity, analyzing its dynamics, parameter estimation, and compatibility with observational data, revealing a transition from deceleration to acceleration consistent with current cosmological observations.
Contribution
The study introduces a specific parametrization of the Hubble parameter in Weyl $f(Q,T)$ gravity and constrains model parameters using observational data, providing new insights into cosmic evolution in this framework.
Findings
Model parameters estimated with MCMC analysis.
Cosmic transition from deceleration to acceleration confirmed.
Model consistent with recent observational data.
Abstract
In the present study, we explore the dynamical characteristics of the quintessence cosmological model in Weyl-type gravity. Here, represents the trace of the matter energy-momentum tensor, and symbolizes the nonmetricity tensor. We propose a solution to the field equation using the specific parametrization in the form, which depicts the necessary transition of cosmos from decelerating era to the current accelerating scenario. The values of model parameters are estimated as , , and using the MCMC analysis and limiting the model with a joint dataset of Pantheon, BAO, and OHD. We discuss the cosmic behavior of many features of the derived model like EoS parameters, energy density, and cosmic pressure. Further, we have also…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Black Holes and Theoretical Physics
