Study of the reconstructed new holographic dark energy F(T, T-G) model

摘要

In this paper, we explore cosmological consequences of the new holographic dark energy model in the background of F(T, T-G) gravity. For this purpose, we consider the reconstruction technique as well as the power-law scale factor. We reconstruct the F(T, T-G) model and investigate its stability by the squared speed of sound parameter. We also discuss the evolution of equation of state, density, deceleration, omega-omega' plane and statefinder parameters. It is found that reconstructed new holographic dark energy F(T, T-G) model is stable for a particular range of b, where b is the constant of the power-law scale factor.