Abstract
In this paper, we study static spherically symmetric wormhole solutions in galactic halo region. Two observational results, Navarro–Frenk–White energy density profile in standard cosmological model and the observed flat rotational curves, are used to discuss traversable wormholes supported by galactic halo in modified Gauss–Bonnet gravity. We explore these solutions either by considering a viable \(f(G)\) model to construct shape function or by specifying the shape function to deduce \(f(G)\) model. We explore energy conditions and find physically acceptable wormhole solutions threaded by normal matter for all values of \(r\). Finally, we investigate stability of the resulting wormhole solutions.
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Sharif, M., Ismat Fatima, H. Wormhole solutions for \(f(G)\) gravity in galactic halo region. Astrophys Space Sci 361, 127 (2016). https://doi.org/10.1007/s10509-016-2715-2
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DOI: https://doi.org/10.1007/s10509-016-2715-2