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A warm inflationary Universe in the Randall-Sundrum II model duringintermediate inflation is studied. For this purpose, we consider a general formfor the dissipative coefficient$\Gamma(T,\phi)=C_{\phi}\,\frac{T^{m}}{\phi^{m-1}}$, and also analyze thisinflationary model in the weak and strong dissipative regimes. We study theevolution of the Universe under the slow-roll approximation and find solutionsto the full effective Friedmann equation in the brane-world framework. In orderto constrain the parameters in our model, we consider the recent data from theBICEP2-Planck 2015 data together with the necessary condition for warminflation $T>H$, and also the condition from the weak (or strong) dissipativeregime.

Warm intermediate inflation in the Randall-Sundrum II model in the light of Planck 2015 and BICEP2 results: A general dissipative coefficient