In f(Q,T) gravity with linear f(Q,T)=αQ+βT and a fitted H(z) parametrization, the model shows a decelerated-to-accelerated transition and thermodynamically viable behavior as an alternative to ΛCDM.
In particular, trajectories approaching the fixed point 12 FIG
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Thermodynamic implications and observational constraints of interacting $f(Q,\mathcal{T})$ gravity in FRW Universe
In f(Q,T) gravity with linear f(Q,T)=αQ+βT and a fitted H(z) parametrization, the model shows a decelerated-to-accelerated transition and thermodynamically viable behavior as an alternative to ΛCDM.