We consider the brane universe in the bulk background of the charged topolo
gical AdS black holes. The evolution of the brane universe is described by
the Friedmann equations for a flat or an open FRW-universe containing radia
tion and stiff matter. We find that the temperature and entropy of the dual
CFT are simply expressed in terms of the Hubble parameter and its time der
ivative, and the Friedmann equations coincide with thermodynamic formulas o
f the dual CFT at the moment when the brane crosses the black hole horizon.
We obtain the generalized Cardy-Verlinde formula for the CFT with an R-cha
rge, for any values of the curvature parameter k in the Friedmann equations
.