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In this paper, we study a warm intermediate inflationary model with a generalform for the dissipative coefficient $\Gamma(T,\phi)=C_\phi\,T^{m}/\phi^{m-1}$in the context of loop quantum cosmology. We examine this model in the weak andstrong dissipative regimes. In general, we discuss in great detail thecharacteristics of this model in the slow-roll approximation. Also, we assumethat the modifications to perturbation equations result exclusively from Hubblerate. In this approach, we use recent astronomical observations from Planck andBICEP2 experiments to restrict the parameters in our model.

General dissipative coefficient in warm intermediate inflation in loop quantum cosmology in light of Planck and BICEP2