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We study warm-tachyon inflationary universe model in the context of theeffective field theory of loop quantum cosmology. In slow-roll approximationthe primordial perturbation spectrums for this model are calculated. We alsoobtain the general expressions of the tensor-to-scalar ratio, scalar spectralindex. We develop this model by using exponential potential, thecharacteristics of this model is calculated in great details. The parameters ofthe model are restricted by recent observational data from Planck, WMAP9 andBICEP2.

Scalar perturbation in warm tachyon inflation in LQC in light of Plank and BICEP2