Structure scalars with charged dissipative systems in [formula omitted] gravity

Abstract

The aim of this investigation is to examine the effect of gravitational modification, in particular, the f(G,T) gravitational field, for dynamically relativistic spherically symmetric systems in the existence of electromagnetic field. The theoretical analysis of dynamical variables linked with charged viscous anisotropic sphere with dissipation is formulated in these environments. We consider that with a relativistic matter, the non-static diagonally symmetric spherical structure is coupled. We linked the Weyl scalar, structure parameters including the charged terms with metric scale factors and mass function. To formulate general form of dynamical variables, we implemented Herrera’s methodology for the orthogonally decomposition of the Riemann tensor. The presence of these variables in the behavioral dynamics of radiating spheres is then analyzed. With the existence and exclusion of fixed f(G,T) values, the parameters essential for the occurrence of inhomogeneities have been studied. It is suggested that with generalized forms of scalar variables, the evolutionary periods of the spherical interiors can be well observed.