An f(Q,C) gravity model with an assumed transit Hubble law is fitted to H(z), supernova, and BAO data, but the fit leaves the model's own parameters unconstrained and unstated.
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Probing Dark Energy Properties in $f Q,C)$ Gravity with FLRW Cosmological Models
An f(Q,C) gravity model with an assumed transit Hubble law is fitted to H(z), supernova, and BAO data, but the fit leaves the model's own parameters unconstrained and unstated.