A Complete Cosmological Scenario in Teleparallel Gravity

Understand

Teleparallel gravity is a modified theory of gravity in which the Ricci scalar $R$ of the Lagrangian replaced by the general function of torsion scalar $T$ in action.

• With that, cosmology in teleparallel gravity becomes profoundly simplified because it is second-order theory.
• The article present a complete cosmological scenario in $f(T)$ gravity with $f(T)=T+\beta(-T)^{\alpha}$, where $\alpha,$ and $\beta$ are model parameters.
• We present the profiles of energy density, pressure, and equation of state (EoS) parameter.