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- W2264664887 abstract "This paper is devoted to study some holographic dark energy models in the context of Chern-Simon modified gravity by considering FRW universe. We analyze the equation of state parameter using Granda and Oliveros infrared cut-off proposal which describes the accelerated expansion of the universe under the restrictions on the parameter α. It is shown that for the accelerated expansion phase $ -1<omega _{Lambda }<-frac {1}{3}$ , the parameter α varies according as $1<alpha <frac {3}{2}$ . Furthermore, for 0<α<1, the holographic energy and pressure density illustrates phantom-like theory of the evolution when ω Λ<−1. Also, we discuss the correspondence between the quintessence, K-essence, tachyon and dilaton field models and holographic dark energy models on similar fashion. To discuss the accelerated expansion of the universe, we explore the potential and the dynamics of quintessence, K-essence, tachyon and dilaton field models." @default.
- W2264664887 created "2016-06-24" @default.
- W2264664887 creator A5005650252 @default.
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- W2264664887 date "2016-09-06" @default.
- W2264664887 modified "2023-10-15" @default.
- W2264664887 title "A Study of Holographic Dark Energy Models in Chern-Simon Modified Gravity" @default.
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- W2264664887 doi "https://doi.org/10.1007/s10773-016-3131-7" @default.
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