Abstract
This paper is devoted to explore some interesting wormhole solutions for the Rastall teleparallel gravity. To complete this analysis, we consider the traceless energy–momentum tensor taken with the Casimir effect concept. Further, we develop two different relations between the pressure components. The anisotropic source of matter with the spherically symmetric space-time is taken to calculate the exact solution, as the shape function. The field equations for Rastall teleparallel gravity are calculated. All the energy conditions are presented for Rastall teleparallel gravity. The presence of exotic matter is confirmed via the violation of energy conditions. All the necessary properties for shape function in all cases are presented graphically. All the inquired results are concluded.
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