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.
On the embedding of spacetime in higher-dimensional spaces with torsion
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abstract
We revisit the Riemann-Cartan geometry in the context of recent higher-dimensional theories of spacetime. After introducing the concept of torsion in a modern geometrical language we present some results that represent extensions of Riemannian theorems. We consider the theory of local embeddings and submanifolds in the context of Riemann-Cartan geometries and show how a Riemannian spacetime may be locally and isometrically embedded in a bulk with torsion. As an application of this result, we discuss the problem of classical confinement and the stability of motion of particles and photons in the neighbourhood of branes for the case when the bulk has torsion. We illustrate our ideas considering the particular case when the embedding space has the geometry of a warped product space . We show how the confinement and stability properties of geodesics near the brane may be affected by the torsion of the embedding manifold. In this way we construct a classical analogue of quantum confinement inspired in theoretical-field models by replacing a scalar field with a torsion field.
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physics.gen-ph 1years
2019 1verdicts
REJECT 1representative citing papers
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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.