Extended gravitational decoupled charged anisotropic solutions

In this paper, we study exact charged anisotropic spherical solutions through extended geometric deformation technique. For this purpose, we consider the singularity-free Krori–Barua solution and extend it to attain two analytical anisotropic models in the presence of the electromagnetic field. We examine energy bounds as well as causality condition for the star Her X-I to analyze the viability of the obtained solutions. It is found that both models show realistic behavior as they satisfy all physical constraints as well as stability criterion. We conclude that the extended gravitational decoupling approach provides more stable results for the stellar system in contrast to minimal geometric deformation.