  In the present work, we investigate the universe dominated by quintom or
hessence energies in Loop Quantum Cosmology (LQC). Interestingly enough, we
find that there are some stable attractors in these two cases. In the case of
quintom, all stable attractors have the feature of decelerated expansion. In
the case of hessence, most of stable attractors have the feature of decelerated
expansion while one stable attractor can have decelerated or accelerated
expansion depend on the model parameter. In all cases, the equation-of-state
parameter (EoS) of all stable attractors are larger than -1 and there is no
singularity in the finite future. These results are different from the dynamics
of phantom in LQC, or the ones of phantom, quintom and hessence in classical
Einstein gravity.
