Analysing Hessence Intermediate and Logamediate Universe in Loop Quantum Cosmological Background

We have discussed here Hessence inflation in Loop Quantum Cosmological background. In this work, we have emphasized on late times, taking into account various slow-roll conditions. This model has been constructed taking intermediate and logamediate scale factors. In both cases the forms of hessence field, potential, number of e-folds, slow-roll parameters are manipulated by taking the dissipative co-efficient Γ =Γ₀, where Γ₀ > 0 is a constant, in accordance with second law of thermodynamics.