Kaniadakis agegraphic dark energy

In this manuscript, we present a novel dark energy scenario based on Kaniadakis entropy, which is generalization of Boltzmann–Gibbs entropy that arises from relativistic statistical theory and characterized by parameter K quantifies the deviations standard expressions, use age Universe as infrared cutoff. The cosmological characteristics proposed model, well evolution cosmos filled with pressure-free matter ensuing candidates, are investigated. interaction non-interaction among two sectors will also be considered. differential equation for density parameter, including expression state deceleration parameters, derived. analysis clearly shows universe to transit decelerated accelerated phase around z≈0.6. most recent 30 H(z) data samples 580 Union 2.1 SNIa set were used limit theoretical results. squared sound speed plotted against redshift z check stability behavior model both cases.