Holographic dark energy through Kaniadakis entropy in non flat universe

Understand

By extending the standard holographic principle to a cosmological framework and combining the non-flat condition with the Kaniadakis entropy, we construct the non-flat Kaniadakis holographic dark energy model.

• The model employs Kaniadakis parameter $K$ and a parameter $c$.
• Derivation of the differential equation for KHDE density parameter to describe the evolutionary behavior of the universe is obtained.
• Such a differential equation could explain both the open as well as closed universe models.