Energy Conditions in Extended $f(R,G,T)$ Gravity

In this paper, we considered the flat Friedmann-Lema\^{i}tre-Robertson-Walker metric in the perspective of perfect fluid models and extended $f(R,G,T)$ gravity (where $R$, $G$ and $T$ are, the Ricci scalar, Gauss Bonnet invariant and the trace of energy momentum tensor, respectively). We focused on specific realistic $f(R,G,T)$ models configuration that could be used to cure finite-time future singularities that arise in late-time cosmic accelerating iterations. We then used the most recent estimated values for the Hubble, deceleration, snap, and jerk parameters to develop the viability and bounds on the models parameters induced by different energy conditions.Comment: 25 pages, 6 figure