English

Standard cosmology from the brane cosmology with a localized matter

High Energy Physics - Theory 2016-09-06 v4

Abstract

We discuss the brane cosmology in the 5D anti de Sitter Reissner-Nordstrom (AdSRN5_5) spacetime. A brane with the tension σ\sigma 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)(\rho_{CFT}) from MM and the charged dust (ρcd2)(-\rho^2_{cd}) from Q2Q^2 in the Friedmann-like equation. However, this equation is not justified because it contains ρcd2\rho_{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 ρdm=\fr32ρcd\rho_{dm}=\fr{\sqrt 3}{2}\rho_{cd}, the unwanted ρcd2-\rho_{cd}^2 is cancelled against ρdm2\rho_{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 ρcstiQ2\rho_{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}=\rho_{sca} to cancel ρcsti-\rho_{csti}. In this case, however, we find a mixed version of the standard and brane cosmologies.

Keywords

Cite

@article{arxiv.hep-th/0103241,
  title  = {Standard cosmology from the brane cosmology with a localized matter},
  author = {Y. S. Myung},
  journal= {arXiv preprint arXiv:hep-th/0103241},
  year   = {2016}
}

Comments

8 pages, Latex, version to appear in MPLA