Role of the brane curvature scalar in the brane world cosmology
arXiv:hep-th/0101091 · doi:10.1016/S0370-2693(01)00236-2
Abstract
We include the brane curvature scalar to study its cosmological implication in the brane world cosmology. This term is usually introduced to obtain the well-defined stress-energy tensor on the boundary of anti de Sitter-Schwarzschild space. Here we treat this as the perturbed term for cosmological purpose. We find corrections to the well-known equation of the brane cosmology. It contains new interesting terms which may play the important role in the brane cosmology.
9 pages, comments and references added, version to appear in PLB
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