Interacting dark energy with CPL admits exact solutions via incomplete gamma functions; Q proportional to dark energy density modestly improves AIC fit but BIC prefers LambdaCDM, showing phantom-to-quintessence transition and possible future transient acceleration.
Interacting dark energy in the early 2020s: A promising solution to theH 0 and cosmic shear ten- sions
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Cosmological evolution of interacting dark energy with a CPL equation of state
Interacting dark energy with CPL admits exact solutions via incomplete gamma functions; Q proportional to dark energy density modestly improves AIC fit but BIC prefers LambdaCDM, showing phantom-to-quintessence transition and possible future transient acceleration.