Anisotropic universe and reconstructing f(R, T) theory from holographic Ricci dark energy

2017 
In this work, we regard f(R, T) gravity as an effective description of the acceleration of the universe and reconstruct the function f(R, T) from the holographic Ricci dark energy by considering a Bianchi type I universe. So the connection gives us an opportunity to redefine the Hubble parameter, the pressure, the equations of state parameter, and the energy density parameter representation by considering Bianchi type I models for holographic Ricci dark energy. We wrap up the evolution of the accelerated expansion of the anisotropic universe, which is faster than the evolution of the FRW and ΛCDM models.
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