arXiv · hep-th/0106245
Brane cosmology with a bulk scalar field
Abstract
We consider ``cosmologically symmetric'' (i.e. solutions with homogeneity and isotropy along three spatial dimensions) five-dimensional spacetimes with a scalar field and a three-brane representing our universe. We write Einstein's equations in a conformal gauge, using light-cone coordinates. We obtain explicit solutions: a. assuming proportionality between the scalar field and the logarithm of the (bulk) scale factor; b. assuming separable solutions. We then discuss the cosmology in the brane nduced by these solutions.
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David Langlois, Maria Rodriguez-Martinez. 2001-06-26. Brane cosmology with a bulk scalar field. https://doi.org/10.1103/physrevd.64.123507
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