arXiv · 2106.04369
Non-exotic wormholes in 4-D Einstein-Gauss-Bonnet gravity
Abstract
In the present paper, we investigate wormholes in 4D-Einstein-Gauss-Bonnet gravity without the requirement of exotic matters. We have taken the radial dependent red-shift function $\phi=\ln \left( {\frac {r_{{0}}}{r}}+1 \right)$ and shape function $b(r)={\frac{r_{0}\ln(r+1)}{\ln({r_0}+1)}}$ as well as anisotropic matter sources through equation of state (EoS) $p_r(r) = \omega \rho(r)$. We examine the energy conditions, flaring out condition, throat condition and anisotropic parameter. The volume integral quantifier is also analyzed to validate the existence and stability of the WH solution. We find, for -ve branch wormhole solutions satisfy the null energy conditions (NEC) throughout the entire space time and +ve branch reduces exactly to Morris-Thorne of GR.
Explore related subjects
Keep this discovery
Ambuj Kumar Mishra, Shweta, Umesh Kumar Sharma. 2021-06-06. Non-exotic wormholes in 4-D Einstein-Gauss-Bonnet gravity. https://doi.org/10.1007/s12043-022-02458-0
Cite the original work for its findings. Save a collection to share your selection of sources.