Strange star with Krori–Barua potential in the presence of anisotropy

In this paper, a well-behaved new model of anisotropic compact star in (3+1)-dimensional spacetime has been investigated the background Einstein’s general theory relativity. The developed by choosing [Formula: see text] component as Krori–Barua (KB) ansatz [Krori and Barua J. Phys. A, Math. Gen. 8 (1975) 508]. field equations have solved proper choice anisotropy factor which is physically reasonable well behaved inside stellar interior. Interior matched smoothly to exterior Schwarzschild vacuum solution it also depicted graphically. Model free from all types singularities static equilibrium under different forces acting on system. stability tested with help various conditions available literature. compatible observed masses radii few stars like Vela X-1, 4U text], PSR J[Formula: LMC X EXO text].