A Study of Holographic Dark Energy Models in Chern-Simon Modified Gravity

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.