M. Hamani Daouda, Manuel E. Rodrigues, M. J. S. Houndjo
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.
View original:
http://arxiv.org/abs/1111.6575
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