Possible existence of wormholes in the galactic halo region
Farook Rahaman, P.K.F. Kuhfittig, Saibal Ray, Nasarul Islam

TL;DR
This paper suggests that the galactic halo's density profile and flat rotation curves could support traversable wormholes, encouraging observational searches for such phenomena in the galaxy.
Contribution
It demonstrates that galactic halo characteristics may naturally support traversable wormholes, linking astrophysical observations with theoretical wormhole models.
Findings
Galactic density profiles can support wormhole structures.
Flat rotation curves are consistent with wormhole-supporting geometries.
Encourages observational efforts to detect galactic wormholes.
Abstract
Two observational results, the density profile from simulations performed in the CDM scenario and the observed flat galactic rotation curves, are taken as input with the aim of showing that the galactic halo possesses some of the characteristics needed to support traversable wormholes. This result should be sufficient to provide an incentive for scientists to seek observational evidence for wormholes in the galactic halo region.
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