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Reconstruction of f(T) gravity according to holographic dark energy
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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 $\Omega_V\rightarrow 1$ at the future time, $\omega_V$ 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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Cited by 1 Pith paper
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Nonlinear reconstruction of general dark energy theories
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