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Possible existence of wormholes in the galactic halo region

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arxiv 1307.1237 v4 pith:FSMOIZ6W submitted 2013-07-04 gr-qc astro-ph.GA

classification gr-qcastro-ph.GA
keywords galactichalowormholesobservationalregioncharacteristicscurvesdensity
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abstract

Two observational results, the density profile from simulations performed in the $\Lambda$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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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Late-Time Cosmology and Structure Formation in Quadratic $f(Q)$ Gravity

    physics.gen-ph 2026-06 unverdicted novelty 4.0 of 10

    Quadratic f(Q) gravity adds an H^4 term to the Friedmann equation and introduces a time-dependent G_eff that suppresses linear growth and halo abundance, offering a modified-gravity route to easing the S8 tension.

  2. Strange quark stars in mimetic gravitational theory

    gr-qc 2025-09 reject novelty 3.0 of 10

    An anisotropic strange quark star model in mimetic gravity is constructed from the Buchdahl metric and MIT bag EoS, with stability checks passed by tuning parameters.

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