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arxiv: hep-th/0104023 · v1 · pith:ZNK6XVSCnew · submitted 2001-04-03 · ✦ hep-th · astro-ph· hep-ph

Cosmological Evolution on Self-Tuned Branes and the Cosmological Constant

classification ✦ hep-th astro-phhep-ph
keywords cosmologicalbraneevolutionpotentialbulkconstantdimensionalfour
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We consider the cosmological evolution of a bulk scalar field and ordinary matter living on the brane world in the light of the constraints imposed by the matter dominated cosmological evolution and a small cosmological constant now. We rule out models with a self-tuned minimum of the four dimensional potential as they would lead to rapid oscillations of the Hubble parameter now. A more natural framework is provided by supergravity in singular spaces where the brane coupling and the bulk potential are related by supersymmetry leading to a four dimensional run-away potential. For late times we obtain an accelerating universe due to the breaking of supersymmetry on the brane with an acceleration parameter of q_0=-4/7 and associated equation of state omega=-5/7.

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