2019/12/16 by M. Abdollahi Zadeh, Zadeh, M. Abdollahi
Computer Science · Physics and Astronomy · #Computational Physics and Python Applications #Cosmology and Gravitation Theories #Statistical Mechanics and Entropy #physics.gen-ph
paper · pdf · doi:10.48550/arxiv.1912.09246
9 pages, 21 figures
arxiv created 2020/01/22 · arxiv updated 2020/01/23
In this paper, we explore various cosmological parameters and cosmological planes (ωD-ωD′, statefinder) for new Tsallis agegraphic dark energy in the framework of Chern-Simons modified gravity. We consider this scenario in a flat FRW universe for both non-interacting and interacting cases, between dark energy and dark matter. It is observed that the equation of state parameter gives quintessence-like nature of the universe in all of the cases. Also, the squared of the sound speed shows unstable behaviour for this scenario. The ωD-ωD′ plane represents the freezing region in most of the cases.