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(similar to)(T) modified theories of gravity. We reconstruct functional forms of f(G) and f(similar to)(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.

Automated summary

In this paper, the cosmic analysis of the Kaniadakis holographic dark energy model is investigated in the frameworks of f(G) and f(similar to)(T) modified theories of gravity. The functional forms of f(G) and f(similar to)(T) models are reconstructed using a power-law form of scale factor and flat FRW metric. The behavior of these functional forms with respect to their arguments is discussed. Various cosmic parameters are explored using these models to discuss the accelerated expansion of the universe, and consistent results are obtained for specific values of model parameters.