Aspects of charged decoupled solutions in R + ΠR2 gravity

This study deals with the physical aspects of the gravitationally decoupled solutions under f(R) gravity scenario. In doing so, charged anisotropic matter composition is assumed as the parent (seed) source for the static spherically symmetric configuration. Commencing with the Kuchowicz ansatz for the charged static parent matter formation, we establish the Karmarkar condition to thoroughly address the deformed functions and the gravitational aspects of the compact spheres. Besides these, null-complexity and isotropized conditions will enforce to grasp the system's stability by the inclusion of charge and R+Pi R-2 factors through graphical trends.