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.
Green Functions for Topology Change
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abstract
We explicitly calculate the Green functions describing quantum changes of topology in Friedman-Lemaitre-Robertson-Walker Universes whose spacelike sections are compact but endowed with distinct topologies. The calculations are performed using the long wavelength approximation at second order in the gradient expansion. We argue that complex metrics are necessary in order to obtain a non-vanishing Green functions and interpret this fact as demonstrating that a quantum topology change can be viewed as a quantum tunneling effect. We demonstrate that quantum topological transitions between curved hypersurfaces are allowed whereas no transition to or from a flat section is possible, establishing thus a selection rule. We also show that the quantum topology changes in the direction of negatively curved hypersurfaces are strongly enhanced as time goes on, while transitions in the opposite direction are suppressed.
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physics.gen-ph 1years
2019 1verdicts
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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.