Abstract

This paper is focused on the investigation of wormhole solutions in [Formula: see text] gravity, where [Formula: see text] denotes the non-metricity scalar. To obtain these solutions, three specific forms of [Formula: see text] gravity models are considered and the shape function, which is responsible for the shape of the wormhole, has been obtained numerically for each model. Further, the energy conditions are checked and the stability of solutions is obtained by determining the adiabatic sound speed in each case.

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