Kaluza-Klein bulk viscous fluid cosmological models and the validity of the second law of thermodynamics in $f(R, T)$ gravity
G. C. Samanta, R. Myrzakulov, Parth Shah

TL;DR
This paper explores Kaluza-Klein cosmological models with bulk viscous fluids in $f(R,T)$ gravity, analyzing thermodynamic laws, and finds conditions under which the second law of thermodynamics holds or is violated.
Contribution
It provides exact solutions for viscous fluid cosmological models in $f(R,T)$ gravity and examines the validity of thermodynamic laws in these models.
Findings
Second law of thermodynamics is violated when viscous coefficient is proportional to $rac{ ext{d}^2a/ ext{d}t^2}{ ext{d}a/ ext{d}t$.
Second law and generalized second law are satisfied when viscous coefficient is proportional to $rac{ ext{d}a}{a}$ or combined forms.
Statefinder parameters differ from $ ext{w}$CDM model, indicating distinct cosmological evolution.
Abstract
The authors considered the bulk viscous fluid in gravity within the framework of Kaluza-Klein space time. The bulk viscous coefficient expressed as , where , and are positive constants. We take , where as an equation of state for perfect fluid. The exact solutions to the corresponding field equations are given by assuming a particular model of the form of , where , is constant. We studied the cosmological model in two stages, in first stage: we studied the model with no viscosity, and in second stage: we studied the model involve with viscosity. The cosmological model involve with viscosity is studied by five possible scenarios for bulk viscous fluid coefficient . The total bulk viscous coefficient…
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