Modeling anisotropic charged neutron star in isotropic coordinates
General Physics
2015-02-12 v1
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.
Cite
@article{arxiv.1502.03378,
title = {Modeling anisotropic charged neutron star in isotropic coordinates},
author = {Ksh. Newton Singh and Narendra Pradhan and Manuel Malaver},
journal= {arXiv preprint arXiv:1502.03378},
year = {2015}
}
Comments
8 pages, 3 figures, 1 table. arXiv admin note: text overlap with arXiv:1410.5808