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Cosmological evolution of interacting dark energy with a CPL equation of state
This paper examines interacting dark energy models within the Chevallier-Polarski-Linder (CPL) parametrization, emphasizing both theoretical structure and observational viability. Two commonly adopted interaction terms are considered: $Q = βH ρ_{de}$ and $Q = βH ρ_c$. We derive exact analytic soluti
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