  A warm inflationary universe scenario on a warped Dvali-Gabadadze-Porrati
brane during intermediate inflation is studied. We consider a general form for
the dissipative coefficient $\Gamma(T,\phi)\propto T^{m}/\phi^{m-1}$, and also
study this model in the weak and strong dissipative regimes. We analyze the
evolution of the universe in the slow-roll approximation, and find the exact
solutions to the equations of motion. In both regimes, we utilize recent data
from the BICEP2 experiment and also from the Planck satellite to constrain the
parameters in our model in accordance with the theory of cosmological
perturbations.
