RECONSTRUCTION OF KANIADAKIS HOLOGRAPHIC DARK ENERGY MODEL IN SELF CREATION THEORY OF GRAVITY

The primary objective of this paper is to examine a Kaniadakis holographic dark energy universe of Bianchi type-II within the framework of self-creation gravity theory. In this dark energy model, the Hubble horizon is used as the infrared cutoff, following Kaniadakis' holographic dark energy concept. We calculate various dynamical parameters in this model, including the statefinder (r, s) plane, the deceleration parameter q, the equation of state (o'de), the square speed of sound, and the o'de - o'' de plane. A graphical analysis of these parameters is provided across a range of free parameter values. The results reveal that the deceleration parameter demonstrates the universe's smooth transition from an early decelerated phase to the current accelerated expansion, while the equation of state parameter suggests a phantom phase. The o'de - o'' de plane reaches the thawing region, and the statefinder plane aligns with both the phantom model and Chaplygin gas. The current values of the parameters are consistent with existing observational data, and the strong energy conditions are found to be violated.