Abstract
This paper is devoted to study the traversable wormhole (WH) solutions in the context of f(đ˘) gravity. For this purpose, we consider the viable power-law form f(đ˘) = ađ˘n as well as specific variable red-shift function and investigate WH geometries for traceless, isotropic as well as barotropic fluids. It is found that in each case, the effective energy-momentum tensor violates the null energy condition throughout the WH throat. We also check the null as well as weak energy conditions for ordinary matter. We conclude that physical acceptable WH solutions exist in certain regions only for radial barotropic case while the range of these regions increases and decreases as the power of đ˘ increases in even and odd manner, respectively.
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