Linear Potentials in Galaxy Halos by Asymmetric Wormholes
A spherically symmetric space-time solution for a diffusive two measures theory is studied. An asymmetric wormhole geometry is obtained where the metric coefficients has a linear term for galactic distances and the analysis of Mannheim and collaborators, can then be used to describe the galactic rot...
Main Authors: | Sebastian Bahamonde, David Benisty, Eduardo I. Guendelman |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2018-10-01
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Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/4/11/112 |
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