Quasi-homologous evolution of relativistic charged objects within f(G, T) gravity

This paper attempts to explore the evolution of relativistic charged (dissipating or non-dissipating) cosmic objects evolving in quasi-homologous (Q(H)) regime and satisfying the condition of zero complexity factor (C-F), under the framework of f(G, T) gravitational theory. For a specific version of f(G, T) theory, various exact solutions for time-dependent charged fluid configurations endowed with spherical symmetry satisfying the above-stated conditions are presented. We will see that few of the provided solutions characterize the evolution of non-static fluid configurations, whose center (r = 0) is enclosed by a void. However, some of the modified solutions exhibit shells and fulfill the Israel junction conditions, while others exhibit voids (i.e., they omit the appearance of shells) and fulfill the Darmois matching conditions on both hypersurfaces. Some future applications regarding the presented models in the field of cosmology and relativistic astrophysics are also mentioned.

Automated summary

This paper explores the evolution of relativistic charged cosmic objects and presents exact solutions satisfying certain conditions. It mentions the potential applications of these models in cosmology and relativistic astrophysics.