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We investigate the warm inflation condition in loop quantum cosmology. In ourconsideration, the system is described by a tachyon field interacted withradiation. The exponential potential function, $V(\phi)=V_0e^{-\alpha\phi}\label{exp-p}$, with the same order parameters $V_0$ and$\alpha$, is taken as an example of this tachyon warm inflation model. We findthat, for the strong dissipative regime, the total number of e-folds is lessthan the one in the classical scenario, and for the weak dissipative regime,the beginning time of the warm inflation will be later than the tachyon (cool)inflation.

A phenomenology analysis of the tachyon warm inflation in loop quantum cosmology