Existence of energy density homogeneity for radiating spheres in f ( G , T ) gravity

This work discusses the responsible quantities of the emergence inhomogeneity by taking locally anisotropic radiating fluid in Formula: see text theory, where T and Formula: see text indicate the trace of stress energy tensor and Gauss–Bonnet terms. The temporal and radial change in mass function is observed with the help of a modified version of Einstein’s field equations. To observe the dynamics of self-gravitating fluid, the dynamical equations and differential equations for conformal tensor are constructed, which help to understand the role of correction terms, Weyl curvature, and fluid parameter in the energy–density irregularity. Various forms of fluid are addressed to meet the desired results.