In this paper, we investigate the effects of electromagnetic field on the isotropic spherical gravastar models in metric $f(R,T)$ gravity. For this purpose, we have explored singularity-free exact models of relativistic spheres with a specific equation of state. After considering Reissner-Nordström spacetime as an exterior region, the interior charged manifold is matched at the junction interface. Several viable realistic characteristics of the spherical gravastar model are studied in the presence of electromagnetic field through graphical representations. It is concluded that the electric charge has a substantial role in the modeling of the proper length, energy contents, entropy, and equation of state parameter of the stellar system. We have also explored the stable regions of the charged gravastar structures.

• Received 25 March 2019
• Revised 26 May 2019

DOI:https://doi.org/10.1103/PhysRevD.100.024062