Modified f (R, G, T) Gravity in the Quintom model, and Inflation

In this paper, I consider a f (R, G, T) modified gravity model where R represents the Ricci scalar, G denotes the Gauss-Bonnet invariant, and T signifies the trace of the stress-energy tensor. This model is coupled with two distinct types of scalar fields. In the flat Friedmann-Lema\^tre-Robertson-Walker (FLRW) universe, the necessary conditions for a successful bounce are achieved. Under these circumstances, it is demonstrated that the equation of state (EoS) parameter cannot cross the phantom divider when only the inflaton scalar field is considered. Appropriate conditions to preserve the conservation of energy law are obtained. The absence of radiation domination is confirmed by referencing one of the collections of the Planck 2018 report. Moreover, it has been demonstrated that this is a general model, encompassing other models such as Weyl conformal geometry and the inflation epoch. Numerical calculations and graphs are used to confirm the results.