Wormhole modeling supported by non-exotic matter

In the present paper, the modeling of traversable wormholes, proposed by Morris and Thorne Am. J. Phys. 56, 395 (1988), is performed within the Formula: see text gravity with particular viable case Formula: see text, where Formula: see text, Formula: see text and Formula: see text. The energy conditions are analyzed using the shape function Formula: see text defined by Godani and Samanta Int. J. Mod. Phys. D 28, 1950039 (2018) and the geometric nature of wormholes is analyzed.