  The braneworld model proposed by Dvali, Gabadadze and Porrati leads to an
accelerated universe without cosmological constant or other form of dark
energy. Nevertheless, we have investigated the consequences of this model when
an holo- graphic dark energy is included, taken the Hubble scale as IR cutoff.
We have found that the holographic dark energy leads to an accelerated universe
flat (de Sitter like expansion) for the two branch: {\ko} = \pm1 of the DGP
model. Nevertheless, in universes with no null curvature the dark energy
presents an EoS corresponding to a phantom fluid during the present era and
evolving to a de Sitter like phase for future cosmic time. In the special case
in which the holographic parameter c is equal to one we have found a sudden
singularity in closed universes. In this case the expansion is decelerating.
Manuscript
