Key points are not available for this paper at this time.
Abstract In this paper, we evaluate the complexity of the anisotropic static cylindrical geometry in the framework of f (G) f (G) gravity, where G G represents the Gauss–Bonnet term. In this perspective, we calculate modified field equations, the C energy formula, the Tolman–Oppenheimer–Volkoff equation, and the mass function that help to understand the astrophysical structures in f (G) f (G) gravity. Furthermore, we used the Weyl tensor and obtained different structure scalars by orthogonally splitting the Riemann tensor. One of these scalars, Yₓ₅ Y TF, is referred to as the complexity factor. This parameter measures system complexity due to non-uniform energy density and non-isotropic pressure. Using the constraint of the variable of vanishing complexity, time-independent solutions are derived for the Gokhroo–Mehra model. It is found that the presence of corrective terms reduce the complexity of the system.
Nasir et al. (Sat,) studied this question.