Anisotropic compact stars in f(T)f(T)f(T) gravity under Karmarkar condition (original) (raw)

In this study, we present a generalized spherically symmetric, anisotropic and static compact stellar model in f(T)f(T)f(T) gravity, where TTT represents the torsion scalar. By employing the Karmarkar condition we have obtained embedding class 1 metric from the general spherically metric of class 2 and the solutions of the Einstein field equations (EFE) has been presented with the choice of suitable parametric values of nnn under a simplified linear form of f(T)f(T)f(T) gravity reads as f(T)=A+BTf(T)=A+BTf(T)=A+BT, where AAA and BBB are two constants. By matching the interior spacetime metric with the exterior Schwarzschild metric at the surface and considering the values of mass and radius of the compact stars we obtain the values of the unknown constants. We have presented further a detailed analysis of the physical acceptability and examined the stability of the stellar configuration by studying the energy conditions, generalized Tolman-Oppenheimer-Volkov (TOV) equation, Herrera cracking concept, adiabatic ...