Standard cosmology from the brane cosmology with a localized matter

preprint2002arXivOpen access

Abstract

We discuss the brane cosmology in the 5D anti de Sitter Reissner-Nordstrom (AdSRN5_5) spacetime. A brane with the tension σσ is defined as the edge of an AdSRN5_5 space with mass MM and charge QQ. In this case we get the CFT-radiation term (ρCFT)(ρ_{CFT}) from MM and the charged dust (−ρcd2)(-ρ^2_{cd}) from Q2Q^2 in the Friedmann-like equation. However, this equation is not justified because it contains ρcd2ρ_{cd}^2-term with the negative sign. This is unconventional in view of the standard cosmology. In order to resolve this problem, we introduce a localized dust matter which satisfies Pdm=0P_{dm}=0. If $ρ_{dm}=\fr{\sqrt 3}{2}ρ_{cd}$, the unwanted −ρcd2-ρ_{cd}^2 is cancelled against ρdm2ρ_{dm}^2 and thus one recovers a standard Friedmann-Robertson-Walker universe with CFT-radiation and dust matter. For the stiff matter consideration, we can set ρcsti∼Q2ρ_{csti}\sim Q^2 with the negative sign. Here we introduce a massless scalar which plays the role of a stiff matter with Psca=ρscaP_{sca}=ρ_{sca} to cancel −ρcsti-ρ_{csti}. In this case, however, we find a mixed version of the standard and brane cosmologies.

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