Central density dependent anisotropic compact stars
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Stars can be treated as a self-gravitating fluid. In this connection, we propose a model for an anisotropic star under the relativistic framework of Krori and Barua (J. Phys. A, Math. Gen. 8:508, 1975) spacetime. It is shown that the solutions are regular and singularity free. The uniqueness of the model is that interior physical properties of the star solely depend on the central density of the matter distribution.
KeywordsDark Energy Central Density Radial Pressure Compact Star Strange Star
MK, FR and SR gratefully acknowledge support from IUCAA, Pune, India under Visiting Associateship Programme under which a part of this work was carried out. SMH is also thankful to IUCAA for giving him an opportunity to visit IUCAA where a part of this work was carried out. FR is personally thankful to PURSE, DST and UGC for providing financial support.