Charged wormhole solutions in f(R) gravity

This study investigates exact charged wormhole solutions within the framework of [Formula: see text] gravity. A viable hyperbolic model is employed to explore the existence of charged wormhole geometries in the presence of relativistic matter configurations. To assess the validity of energy conditions, a specific matter form and a combination of shape functions are analyzed. The analysis is conducted within the context of a static, spherically symmetric space-time. An anisotropic fluid idea was used to evaluate the equilibrium backdrop of a charge wormhole model, and our results were graphically explored. The gravitational entity that resulted from [Formula: see text] gravity in the form of extra-curvature quantities further validated these non-standard astrophysical wormhole ideas. In addition, it was shown that the charge wormhole model might exist in specific regions of the parameter space without the need for exotic matter, provided that an anisotropic fluid is present and [Formula: see text], gravity.