Anisotropic effect on barrow holographic dark energy

In this paper, we investigate a non-interacting model considering a spatially anisotropic and homogeneous Bianchi type-I Universe, filled with Barrow holographic dark energy (BHDE) and pressureless dark matter. We examine some important cosmological parameters for the evolutionary report and to witness adequate nature in BHDE model as including deceleration parameter, the jerk parameter, equation of state parameter and density parameter. To study more briefly, we diagnose statefinder parameters, omega(D) - omega(D)' analysis and explain that the model parameter significantly modifies the evolutionary trajectories in these planes.