Brane cosmology with a bulk scalar field
arXiv:hep-th/0106245 · doi:10.1103/PhysRevD.64.123507
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.
24 pages, Latex, no figure
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Cited by in corpus (52)
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