On relativistic anisotropic compact stars
Ksh. Newton Singh, M. V. Mandke, Anil K. Aria
DOI Number:
Class one solution, Compact stars, General Relativity, Stability
In the present article we provide a new model of compact star satisfying the Karmarkar condition. We proceed our calculations by assuming a new type of metric potential for g_rr and g_tt is obtained from the condition of embedding class one. The physical parameters are obtained by employing the metric potentials to the Einstein’s field equations. Our model is free from central singularity and satisfies all the physical conditions. We have also investigated equilibrium and stability of compact star by several methods.
Article Details
Unique Paper ID: 150947

Publication Volume & Issue: Volume 7, Issue 11

Page(s): 61 - 65
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