Study of cosmic acceleration in modified theories of gravity through Kaniadakis holographic dark energy.

In this paper, we investigate the cosmic analysis of Kaniadakis holographic dark energy model in the frameworks of f (G) and f ̃ (T) modified theories of gravity. We reconstruct functional forms of f (G) and f ̃ (T) models by using a well-known power-law form of scale factor and flat FRW metric. The behavior of these functional forms with respect to their arguments is discussed. Using these models, various cosmic parameters like energy conditions, effective equation of state parameter, deceleration parameter and squared speed of sound parameters are explored to discuss the accelerated expansion of the universe. We obtain some consistent results for accelerated expansion of the universe related to specific values of model parameters. [ABSTRACT FROM AUTHOR]