All spherically symmetric charged anisotropic solutions for compact star
arXiv:1502.01915 · doi:10.1140/epjc/s10052-017-4917-3
Abstract
In the present paper we develop an algorithm for all spherically symmetric anisotropic charged fluid distribution. Considering a new source function we find out a set of solutions which is physically well behaved and represent compact stellar models. A detailed study specifically shows that the models actually correspond to strange stars in terms of their mass and radius. In this connection we investigate about several physical properties like energy conditions, stability, mass-radius ratio, electric charge content, anisotropic nature and surface redshift through graphical plots and mathematical calculations. All the features from these studies are in excellent agreement with the already available evidences in theory as well as observations.
28 pages, 15 figures, major changes in the text. arXiv admin note: text overlap with arXiv:1408.5126 by other authors
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- Generating solutions for charged stellar models in general relativity
- A generalized Finch-Skea class one static solution
- Stellar Structures in Gravity with Tolman-Kuchowicz Spacetime
- Durgapal IV model in light of the minimal geometric deformation approach
- Relativistic compact stars with charged anisotropic matter
- Modeling of charged anisotropic compact stars in general relativity
- Relativistic Polytropic Models of Charged Anisotropic Compact Object
- Exact solution of anisotropic compact stars via. mass function