  Holographic dark energy models have proven to be a very interesting way to
study various aspects of late-time acceleration of the universe. In this work
we extensively study HDE models with the Granda-Oliveros cutoff with an ansatz
based approach. We consider the Tsallis, Barrow and PLEC HDE models in this
regard and consdier simple power law, emergent universe, intermediate and
logamediate forms of for the universe. Studying various cosmologically
interesting parameters alongside the thermodynamical aspects in these models,
we show that the Logamediate models are the best fit out of the other
possibilites, followed by the emergent universe model, intermediate model and
the simple power law models at the very last in terms of feasibility.
