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Thermodynamic reconstruction in observationally constrained dynamical dark energy models
We perform an observational and thermodynamic analysis of four cosmological models $Λ$CDM, CPL, MPL, and the three-parameter MmAH parametrization. All dynamical models improve the fit relative to $Λ$CDM, with $Δχ^2 \sim 6$-$6.5$, with MPL providing the best fit, while MmAH remains viable. Although B
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