arXiv · 1907.07344
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 $f(R)=R-\mu R_c\Big(\frac{R}{R_c}\Big)^p$, 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.
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Gauranga C. Samanta, Nisha Godani. 2019-07-17. Wormhole Modeling Supported by Non-Exotic Matter. https://doi.org/10.1142/s0217732319502249
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