Reconstruction of f(T) gravity according to holographic dark energy
Abstract
We develop the reconstruction of a model of f(T) gravity according to the holographic dark energy. T is the torsion scalar and its initial value from the Teleparallel gravity is imposed for fitting the initial value of the function f(T). The result shows a polynomial function for f(T), and we also observe that, when V→ 1 at the future time, ωV may cross -1 for some values of the input parameter b. Another interesting aspect of the obtained model is that it provides the unification of the dark matter with the dark energy.
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