  We discuss the brane cosmology in the 5D anti de Sitter Reissner-Nordstrom
(AdSRN$_5$) spacetime. A brane with the tension $\sigma$ is defined as the edge
of an AdSRN$_5$ space with mass $M$ and charge $Q$. In this case we get the
CFT-radiation term $(\rho_{CFT})$ from $M$ and the charged dust
$(-\rho^2_{cd})$ from $Q^2$ in the Friedmann-like equation.
  However, this equation is not justified because it contains
$\rho_{cd}^2$-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 $P_{dm}=0$. If $\rho_{dm}=\fr{\sqrt
3}{2}\rho_{cd}$, the unwanted $-\rho_{cd}^2$ is cancelled against $\rho_{dm}^2$
and thus one recovers a standard Friedmann-Robertson-Walker universe with
CFT-radiation and dust matter. For the stiff matter consideration, we can set
$\rho_{csti}\sim Q^2$ with the negative sign. Here we introduce a massless
scalar which plays the role of a stiff matter with $P_{sca}=\rho_{sca}$ to
cancel $-\rho_{csti}$. In this case, however, we find a mixed version of the
standard and brane cosmologies.
