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The emergent model in the context of loop quantum cosmology with a tachyonscalar field is studied. We find that there is a center equilibrium point inthe semiclassical region and a saddle point in the classical region. If thepotential of the tachyon field satisfies some conditions, the universe can stayat the center equilibrium point past-eternally and then oscillate infinitelyaround this point with the tachyon climbing up its potential. Once thepotential reaches a critical value, these two equilibrium points coincide witheach other and the oscillation phase is broken by an emergent inflation. Inorder to obtain a successful emergent tachyon inflation, a constraint on$\dot{\phi}^2$ of tachyon is required.

Inverse volume corrections to emergent tachyonic inflation in loop quantum cosmology