A comparative analysis of self-consistent charged anisotropic spheres

This study is devoted to exploring the charged stellar structures under embedded space-time using the Karmarkar condition. For this, spherically symmetric space-time with the anisotropic source of fluid possessing an electric charge has been incorporated. Further, the Bardeen and Reissner-Nordstrom geometries have been employed as exterior space-time to calculate the values of the involved constants. The interior solutions of a stellar object have been worked out with the observational mass M = 2.01M(circle dot), and R-epsilon = 9.1 km. It is argued that the acquired solutions accomplish all the necessary conditions for self-consistent charged stars. It has been noted through the detailed graphical analysis that our obtained solutions are physically stable and self-consistent with the best degree of accuracy for n is an element of [12, 15], where parameter n is involved in the model under discussion. Beyond this bound 12 <= n <= 15, the realistic solutions of stellar models under discussion could not be found. After perceiving the marginal dissimilarities between our proposed models in both cases, Andreasson's limit root R-epsilon/3 + root R-epsilon/9 + q(2)/3R(epsilon)>= root M, critically important for the stellar structures, has been achieved in both the models under investigation. Lastly, it is established that the parameter n has a substantial effect on worked-out solutions under the employment of Bardeen and Reissner-Nordstrom's stellar structures.