Dynamical conditions and causal transport of dissipative spherical collapse in f(R, T) gravity

In this paper, we have investigated the non-adiabatic spherical gravitational collapse in framework of $f(R,T)$ theory gravity with a locally anisotropic fluid that undergoes dissipation form heat flux, free-streaming radiation, and shearing viscosity. The dynamical equations are analyzed detail, both Newtonian post-Newtonian regimes. Finally couple to full causal transport equation context Israel-Stewart dissipative systems. This yields us better understanding dynamics may be connected various astrophysical consequences.