2024/05/11 by Oem Trivedi, Maxim Khlopov, Trivedi, Oem +1
Computer Science · Physics and Astronomy · Earth and Planetary Sciences · #Computational Physics and Python Applications #Cosmology and Gravitation Theories #Geophysics and Gravity Measurements
paper · pdf · doi:10.48550/arxiv.2405.15798
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.