A dipolar dark matter model with a non-Abelian SU(2) internal force reproduces the deep-MOND regime without arbitrary functions, but the MOND scale depends on free and galaxy-specific parameters.
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Dipolar dark matter theory based on a non-Abelian Yang-Mills field
A dipolar dark matter model with a non-Abelian SU(2) internal force reproduces the deep-MOND regime without arbitrary functions, but the MOND scale depends on free and galaxy-specific parameters.