Embedded Interior Solutions Of V Ela X-1 Model In F(Tau, T) Gravity

This article is based on the extension of Teleparallel Theory named f(tau, T) gravity, where the notions tau and T abbreviate the torsion trace term of the energy-momentum tensor. This study aims to explore the anisotropic outcomes of the V ela X - 1 model. We use the field equations drawn by using the spherical symmetry, including the torsion trace term. The major components g(rr) and g(tt), of spherical symmetric space-time are obtained by inducing the Karmarkar condition. We can obtain the values of the involved parameters c,P, Q in this study by matching the interior spherical metric with the exterior Schwarzschild's solutions of the Einstein field equations. To explore the stability of the stellar objects predicted by our study, we study the properties like metric potentials, energy density, pressures, anisotropy, gradients, EoS, energy conditions, the behavior of forces, sound speeds, adiabatic index, redshift, mass function, and compactification by graphical analysis in the background of f(tau, T) gravity.