Structure Scalars for Charged Dissipative Spherical Collapse in $f(R, T)$ Gravity

In this paper, we examine the structure scalars formed from the orthogonal splitting of the Riemann tensor of the spacetime metric describing the interior of a charged matter configuration undergoing dissipative collapse in $f(R,T)$ gravity, and how they influence the various physical parameters of the collapsing matter. A treatment is provided for the unspecified $f(R, T)$ function, and the nature of the results for a linear $f(R, T)$ function is presented. In the absence of dissipation, the energy density inhomogeneity is influenced by $X_{TF}$ and the mass function. Further, the presence of charge affects the structure scalars and the total mass-energy content. The dependence of various physical parameters, such as heat dissipation, energy density inhomogeneity, evolution of the expansion scalar, the shear scalar, effective homogeneous energy density, and pressure anisotropy, on the structure scalars has been clearly indicated.