Linear potentials in galaxy halos by Asymmetric Wormholes

Abstract

A spherically symmetric space-time solution for a diffusive two measures theory is studied. An asymmetric wormhole geometry is obtained where the metric coefficients have a linear term for galactic distances and the analysis of Mannheim and collaborators, can then be used to describe the galactic rotation curves. For cosmological distances, a de-Sitter space-time is realized. Centre of gravity coordinates for the wormhole is introduced which are the most suitable for the collective motion of a wormhole. The wormholes connect universes with different vacuum energy densities which may represent different universes in a "landscape scenario". The metric coefficients depend on the asymmetric wormhole parameters. The coefficient of the linear potential is proportional to both the mass of the wormhole and the cosmological constant of the observed universe. Similar results are also expected in other theories like $k$-essence theories, that may support wormholes.

arXiv commentSome small changes. Matches the published version in Universe

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Cited by in corpus (6)

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• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Fate of a Thin-Shell Wormhole Powered by Morris-Thorne Wormhole
• The Stability of Asymmetric Cylindrical Thin-Shell Wormholes
• The Local Group as a test system for Modified Newtonian Dynamics
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