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We construct a holographic dark energy scenario based on Kaniadakis entropy,which is a generalization of Boltzmann-Gibbs entropy that arises fromrelativistic statistical theory and is characterized by a single parameter $K$which quantifies the deviations from standard expressions, and we use thefuture event horizon as the Infrared cutoff. We extract the differentialequation that determines the evolution of the effective dark energy densityparameter, and we provide analytical expressions for the correspondingequation-of-state and deceleration parameters. We show that the universeexhibits the standard thermal history, with the sequence of matter anddark-energy eras, while the transition to acceleration takes place at$z\approx0.6$. Concerning the dark-energy equation-of-state parameter we showthat it can have a rich behavior, being quintessence-like, phantom-like, orexperience the phantom-divide crossing in the past or in the future. Finally,in the far future dark energy dominates completely, and the asymptotic value ofits equation of state depends on the values of the two model parameters.

Kaniadakis holographic dark energy and cosmology