Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates
International Journal of Astrophysics and Space Science
Volume 3, Issue 1-1, February 2015, Pages: 13-20
Received: Nov. 17, 2014; Accepted: Nov. 19, 2014; Published: Dec. 19, 2014
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Authors
Ksh. Newton Singh, Department of Physics, National Defence Academy, Khadakwasla, Pune-411023, India
Narendra Pradhan, Department of Physics, National Defence Academy, Khadakwasla, Pune-411023, India
Manuel Malaver, Department of Basic Sciences, Maritime University of the Caribbean, Catia la Mar, Venezuela
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Abstract
We present a spherically symmetric solution of the general relativistic field equations in isotropic coordinates for charged fluid with pressure anisotropy, compatible with a super dense star modeling. Further, we have constructed an anisotropic model of super dense star with all degree of suitability. We also observed that by increasing anisotropy, the maximum mass of super dense stars also decreases.
Keywords
Isotropic Coordinates, Charged Fluid, Anisotropic Model, Super Dense Star
To cite this article
Ksh. Newton Singh, Narendra Pradhan, Manuel Malaver, Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates, International Journal of Astrophysics and Space Science. Special Issue:Compact Objects in General Relativity. Vol. 3, No. 1-1, 2015, pp. 13-20. doi: 10.11648/j.ijass.s.2015030101.13
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