Wormhole modeling supported by non-exotic matter
Abstract
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−μRc(RRc)p, where μ, Rc>0 and 0<p<1. The energy conditions are analyzed using the shape function b(r)=rlog(r+1)log(r0+1) defined by Godani and Samanta [Int. J. Mod. Phys. D28, 1950039 (2018)] and the geometric nature of wormholes is analyzed.