Cosmic aspects of specific dark energy model in loop quantum cosmology

We consider the interacting scenario of pilgrim dark energy (with future event horizon) with cold dark matter in loop quantum cosmology. We explore various cosmological parameters (Hubble, equation of state and deceleration) and planes ([Formula: see text] and [Formula: see text]–[Formula: see text]) in this framework. We also discuss the validity of generalized second law of thermodynamics and find that it remains valid in the early epoch as well as in late future epoch. Finally, it is remarked that all the above constraints of cosmological parameters show consistency with different observational data like Planck, WP, BAO, [Formula: see text], SNLS and nine-year WMAP.

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