Analytical stellar models of neutron stars in teleparallel gravity

In this paper, we developed three analytical models and obtained a new class of solutions describing compact stellar structures using the theory teleparallel gravity. We consider general anisotropic nature configurations solve gravity equations. order to thoroughly analyze various parameters stars, by choosing physically acceptable forms metric potential $ e^{d(r)} radial pressure p_r(r) $. also impact gravity's \beta \beta_1 on description structures. calculated model such that observed neutron stars obey all physical conditions be potentially stable causal. By analyzing structures, found in paper can describe ranging from low density high density. Finally, obtain quadratic Equation State for each which utilized find compositions It is very useful exhibit EOS, since material real strange are EOS authors. Non linear f(T) gives deviation behaviour, thus, work with function diagonal tetrad realistic stars.