Evolution of the charged dynamical radiating spherical structures

In the scenario of f(R, T, Q) gravity, where R and T represent the Ricci scalar and the trace of stress energy tensor respectively, and Q equivalent to R mu nu T mu nu, we generalize the concept of complexity for dissipative dynamical spherically self-gravitating fluid configuration proposed by Herrera et al. (2018). As the fluid contains dynamical situation, we evaluate the structural complexity as well as the complexity of the pattern of evolution for matter configuration in the presence of electric charge and check their viability under f(R, T, Q) correction terms. In the context of modified gravity, we calculate some dynamical and kinematical equations in both dissipative and nondissipative phenomena. Eventually, we construct the equations for the structural scalars evolution and consistency of the condition at which the complexity factor disappears. For f(R, T, Q) = R in modified action, all of our results reduce to general relativity. (c) 2020 Elsevier Inc. All rights reserved.