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- W2949969144 abstract "Recently, Tsallis, R'{e}nyi and Sharma-Mitall and entropies have widely been used to study the gravitational and cosmological setups. We consider a flat FRW universe with linear interaction between dark energy and dark matter. We discuss the dark energy models using Tsallis, R'{e}nyi and Sharma-Mitall entropies in the framework of Chern-Simons modified gravity. We explore various cosmological parameters (equation of state parameter, squared sound of speed ) and cosmological plane ($omega_{d}-omega_{d}'$, where $omega_{d}'$, is the evolutionary equation of state parameter). It is observed that the equation of state parameter gives quintessence-like nature of the universe in most of the cases. Also, the squared speed of sound shows stability of the models for Tsallis, R'{e}nyi dark energy model while unstable behavior for Sharma-Mitall dark energy model. The $omega_{d}-omega_{d}'$ plane represents the thawing region for all dark energy models." @default.
- W2949969144 created "2019-06-27" @default.
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- W2949969144 date "2018-12-20" @default.
- W2949969144 modified "2023-09-27" @default.
- W2949969144 title "Cosmological Implications of the Generalized Entropy Based Holographic Dark Energy Models in Dynamical Chern-Simons Modified Gravity" @default.
- W2949969144 cites W3102249952 @default.
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- W2949969144 doi "https://doi.org/10.48550/arxiv.1901.01311" @default.
- W2949969144 hasPublicationYear "2018" @default.
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