  We study warm-tachyon inflationary universe model in the context of the
effective field theory of loop quantum cosmology. In slow-roll approximation
the primordial perturbation spectrums for this model are calculated. We also
obtain the general expressions of the tensor-to-scalar ratio, scalar spectral
index. We develop this model by using exponential potential, the
characteristics of this model is calculated in great details. The parameters of
the model are restricted by recent observational data from Planck, WMAP9 and
BICEP2.
