Research PaperNo Access

Electric and Energy Department, Tunceli Vocational School, Munzur University, Tunceli 62000, Turkey

https://doi.org/10.1142/S0217751X22502141Cited by:5 (Source: Crossref)

Abstract

In this work, considering anisotropic and homogeneous Bianchi type-V universe we investigated Kaniadakis holographic dark energy (KHDE). It is demonstrated that the equation of state (EoS) parameter has a transition from the quintessence era to the phantom era for the chosen model. Additionally, in the late time of the universe, EoS parameter behaves like a cosmological constant ( $Λ$ ) with an IR (Infrared) cut-off apparent horizon in case of a particular form of deceleration parameter. We reconstructed correspondence between the KHDE and tachyon, quintessence and k-essence scalar fields. Also, our numerical solutions have been shown in graphs for EoS parameter and scalar fields.

Keywords:

PACS: 98.80.−k, 95.36.+x

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