Abstract
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.
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Mandal, J.D., Debnath, U. Analysing Hessence Intermediate and Logamediate Universe in Loop Quantum Cosmological Background. Int J Theor Phys 56, 1771–1783 (2017). https://doi.org/10.1007/s10773-017-3324-8
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DOI: https://doi.org/10.1007/s10773-017-3324-8