Bulk viscous cosmological model in $f(T,\mathcal{T})$ modified gravity
Raja Solanki, Aaqid Bhat, P.K. Sahoo

TL;DR
This paper investigates how bulk viscosity influences the accelerated expansion of the universe within a modified $f(T,\
Contribution
It introduces and analyzes specific $f(T,\
Findings
Models fit observational data well
Linear model mimics $\\Lambda$CDM
Effective EoS indicates acceleration
Abstract
This article explores the impact of bulk viscosity on understanding the universe's accelerated expansion within the context of modified gravity, which is an extension of the gravitational theory, allowing a broad coupling between the energy-momentum scalar and the torsion scalar . We consider two functions, specifically and , where and are arbitrary constants, along with the fluid part incorporating the coefficient of bulk viscosity . We calculate the analytical solutions of the corresponding field equations for a flat FLRW environment, and then we constrain the free parameters of the obtained solution using CC, Pantheon+, and the CC+Pantheon+ samples. We perform the Bayesian statistical…
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