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We investigate the observational signatures of quantum cosmology in theCosmic Microwave Background data provided by Planck collaboration. We apply thewarm inflationary paradigm with a tachyon scalar field to the loop quantumcosmology. In this context, we first provide the basic cosmological functionsin terms of the tachyon field. We then obtain the slow-roll parameters and thepower spectrum of scalar and tensor fluctuations respectively. Finally, westudy the performance of various warm inflationary scenarios against the latestPlanck data and we find a family of models which are in agreement with theobservations.

Tachyon warm inflation with the effects of Loop Quantum Cosmology in the light of Planck 2015