Cosmological constraints in symmetric teleparallel gravity with bulk viscosity
Dheeraj Singh Rana, P.K. Sahoo

TL;DR
This paper investigates the accelerated expansion of the universe using a modified $f(Q)$ gravity model with bulk viscosity, deriving analytical solutions and fitting them to observational data to support a quintessence-like late-time acceleration.
Contribution
It introduces a bulk viscous cosmological model within $f(Q)$ gravity, providing analytical solutions and observational constraints, highlighting the role of viscosity in cosmic acceleration.
Findings
The model predicts accelerated expansion consistent with observations.
The viscous model favors quintessence-type dark energy behavior.
Analytical solutions fit well with combined observational data.
Abstract
In this study, we explore the accelerated expansion of the universe within the framework of modified gravity. The investigation focus on the role of bulk viscosity in understanding the universe's accelerated expansion. Specifically, a bulk viscous matter-dominated cosmological model is considered, with the bulk viscosity coefficient expressed as . We consider the power law function , where and are arbitrary constants and derive the analytical solutions for the field equations corresponding to a flat FLRW metric. Subsequently, we used the combined Cosmic Chronometers (CC)+Pantheon+SH0ES sample to estimate the free parameters of the obtained analytic solution. We conduct Bayesian statistical analysis to estimate the posterior probability by employing the likelihood function and the MCMC random sampling…
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