Wormhole Modeling Supported by Non-Exotic Matter

In the present paper, the modelling of traversale wormholes, proposed by Morris & Thorne \cite{morris1}, is performed within the $f(R)$ gravity with particular viable case $f(R)=R-\mu R_c(\frac{R}{R_c}{)}^p$, where $\mu, R_c>0$and$0<p<1$\mathrm{.}Theenergyconditionsareanalyzedusingtheshapefunction$b®=\frac{r\log(r+1)}{\log(r_0+1)}$ defined by Godani and Samanta \cite{godani} and geometric nature of wormholes is analyzed.