Complexity of Dynamical Dissipative Cylindrical System in Non-minimally Coupled Theory

Abstract

This paper aims to formulate certain scalar factors associated with matter variables for self-gravitating non-static cylindrical geometry by considering a standard model $\mathcal{R}+\zeta \mathcal{Q}$ of $f(\mathcal{R},\mathcal{T},\mathcal{Q})$ gravity, where $\mathcal{Q}={\mathcal{R}}_{\phi \vartheta }{\mathcal{T}}^{\phi \vartheta }$ and $\zeta$ is the arbitrary coupling parameter. We split the Riemann tensor orthogonally to calculate four scalars and deduce ${\mathcal{Y}}_{TF}$ as complexity factor for the fluid configuration. This scalar incorporates the influence of inhomogeneous energy density, heat flux and pressure anisotropy along with correction terms of the modified gravity. We discuss the dynamics of cylinder by considering two simplest modes of structural evolution. We then take ${\mathcal{Y}}_{TF}=0$ with homologous condition to determine the solution for dissipative as well as non-dissipative scenarios. Finally, we discuss the criterion under which the complexity-free condition shows stable behavior throughout the evolution. It is concluded that complex functional of this theory results in a more complex structure.

arXiv comment27 pages, no figure

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