2000
DOI: 10.1016/s0370-2693(00)00850-9
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Standard cosmology from sigma-model

Abstract: We investigate (4+1)-and (5+0)-dimensional gravity coupled to a non-compact scalar field sigma-model and a perfect fluid within the context of the Randall-Sundrum scenario. We find cosmological solutions with a rolling fifth radius and a family of warp factors. Included in this family are both the original Randall-Sundrum solution and the self-tuning solution of Kachru, Schulz and Silverstein. Our solutions exhibit conventional cosmology.

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Cited by 9 publications
(11 citation statements)
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“…[15]. However, there has been little, and only very recent, work on the cosmology of automatically Poincare invariant branes [16].…”
mentioning
confidence: 99%
“…[15]. However, there has been little, and only very recent, work on the cosmology of automatically Poincare invariant branes [16].…”
mentioning
confidence: 99%
“…In order to explore the transition between an accelerating universe and matter domination we need to consider the bulk solution in a perfect fluid. For example, [11] has considered a self-tuned domain wall in five dimensional gravity coupled to a scalar field with bulk fluid, obtaining matter dominated FRW dynamics induced on the brane. Coupling this to our mechanism for an accelerating universe should result in a rich cosmology, such as a modified Friedmann equation on the brane-world.…”
Section: Discussionmentioning
confidence: 99%
“…Notice that these conditions are automatically satisfied due to the assignment (11). The equations of motion can be written in BPS form…”
Section: Cosmological Solutionsmentioning
confidence: 99%
“…We make the ansatz that both the potentials U and V are of Liouville type: (6) and that the metric is:…”
Section: The Modelmentioning
confidence: 99%
“…The wormhole is time-dependent and the bounce involves the entire Universe. Our analysis will be along the lines of the one in [6].…”
Section: Introductionmentioning
confidence: 99%