  In the background of a charged AdS dilaton black hole, we investigate the
movement of a self-graviting 3-brane and relevant holographic effects as the
brane move close to the AdS boundary. The induced metric on brane corresponds
to an exact FLRW geometry, while the evolution of brane is determined by Israel
junction condition and the effective Einstein field equation on brane together.
When the brane approaches the AdS boundary, AdS/CFT correspondence implies that
a radiation dominated FLRW-universe ($P=\frac{1}{3}\rho$) should be given.
According to the holographic renormalization procedure, we involve an
appropriate surface counterterm into the gravitational action for achieving
$P=\frac{1}{3}\rho$ on brane. This surface counterterm also plays a important
role in caculating the mass of charged AdS dilaton black hole. Finally, we
obtain the thermodynamic quantities and give an extend Cardy-Verlinde formula
on brane.
