Traversable Wormhole Geometry Reconstruction from the Rotation Curve of NGC 3198: A Comparative Study of Dark Matter Halo Profiles
By reconstructing a traversable wormhole metric directly from the observed rotation curve of the spiral galaxy NGC 3198 using four dark matter halo profiles, this study demonstrates that the observationally favored Burkert profile not only provides the best fit to the data but also satisfies the geometric requirements for a traversable wormhole while exhibiting the necessary exotic matter characteristics near the galactic center.