Dark matter is modeled as same-sign dark charges at the ends of Kalb-Ramond strings, and the standard isothermal halo density profile is shown to be an exact Einstein-Maxwell charged dust solution, though the profile is imposed rather than derived.
Isothermal spheres and charged dust
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Strings, Topological Change and Dark Matter
Dark matter is modeled as same-sign dark charges at the ends of Kalb-Ramond strings, and the standard isothermal halo density profile is shown to be an exact Einstein-Maxwell charged dust solution, though the profile is imposed rather than derived.