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 f(R) gravity with particular viable case f(R) = R - mu R-c(R/R-c)(p) where mu, R-c > 0 and 0 < p < 1. The energy conditions are analyzed using the shape function b(r) = r log(r+ 1)/log(r(0)+1) defined by Godani and Samanta [Int. J. Mod. Phys. D 28, 1950039 (2018)] and the geometric nature of wormholes is analyzed.