Bardeen strange stellar structures

Abstract

This study is explored to discuss the anisotropic nature of charged strange compact stars by considering the MIT bag model in the context of our universe’s accelerated expansion scenario. For this purpose, we choose two models for spherically symmetric space–time components. In Model-I, we plug the embedded space–time to evaluate the Bardeen strange stellar structures. In Model-II, we choose the Krori–Barua space–time. We correlate the Bardeen geometry as an exterior solution with a spherically symmetric interior geometry to acquire unknown parameters involved in the study. We discuss the necessary properties of the strange stellar models with embedded space–time and Krori–Barua space–time via the MIT bag model. After witnessing the minor differences in our proposed models, Andreasson’s limit [Formula: see text] has been fulfilled as required by the charged stellar structures. Further, we conclude that all the acquired results show the stable and self-consistent behavior of charged anisotropic compact structures.