Non-exotic wormhoe in Rastall theory

This paper examines exact wormhole solutions within the framework of Rastall theory. Given that the Einstein field equations are altered in 3+1 dimensions under Rastall’s gravitational theory, we have explored potential solutions utilizing various forms of the equation of state. The influence of the Rastall parameter on the null energy condition, a crucial aspect of wormholes, is analyzed. Additionally, asymptotic flatness is highlighted as a significant characteristic of these solutions. We also address several physical and mathematical properties associated with these solutions. This document presents a comparative analysis of wormhole solutions within the framework of Rastall gravity, in contrast with f ( T , T ) as a teleparallel formulation of general relativity and f ( R, T ) as a curvature-based gravity.