Wormhole Modeling Supported by Non-Exotic Matter

Abstract

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 $0<p<1$. The energy conditions are analyzed using the shape function $b(r)=\frac{r\log (r+1)}{\log (r_0+1)}$ defined by Godani and Samanta \cite{godani} and geometric nature of wormholes is analyzed.

arXiv comment14 pages, 8 figures, to be appear in Modern Physics Letters A

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