Possible existence of charged traversable wormholes in f(R,T) gravity with strange matter content

In this study, we explore the geometric features of a charged traversable wormhole (WH) in the realm of [Formula: see text] gravity with strange quark matter. We developed the field equations for Morris–Thorne-type charged WH metric with anisotropic fluid distribution and obtained the corresponding WH results for two kinds of shape functions. To visualize the proper shape of the WH, we depicted three-dimensional and two-dimensional embedding portraits for the chosen values of both [Formula: see text] and [Formula: see text] at the throat radius [Formula: see text]. In addition, all necessary needs to build a WH shape are analyzed for the considering shape functions. Next, we analyze the energy conditions together with the MIT bag model, for different values of free parameters for both cases. It is observed that in both cases, all the energy conditions are violated in different regions of the WH spacetime, corresponding to some ranges of model parameters. The violation of the null energy condition (NEC) confirms the existence of exotic matter inside the WH throat. On the other hand, the validity of energy conditions predicts a fabric of stable traversable WHs. For both cases, the equilibrium configuration is analyzed through the TOV equation showing the stability of considering solutions.