Holographic dark energy reconstruction in (Formula presented.)gravity

The present paper reports a holographic reconstruction scheme for f(T,T) gravity proposed in Harko et al. (J. Cosmol. Astropart. Phys. 12:021, 2014), where T is the torsion scalar and T is the trace of the energy-momentum tensor considering future event horizon as the enveloping horizon of the universe. We consider f(T,T)=T+γg(T) and f(T,T)=βT+g(T) for reconstruction. We also extract the equation of state parameter for these models. We also give the comparison of the results with observational data and found the consistency of our results.