Closed form charged fluid with t = constant hypersurfaces as spheroids and hyperboloids

Details Closed form charged fluid with t = constant hypersurfaces as spheroids and hyperboloids Closed form charged fluid with t = constant hypersurfaces as spheroids and hyperboloids

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.337..455b&link_type=abstract

Astrophysics and Space Science, Volume 337, Issue 1, pp.455-462

Astronomy and Astrophysics

Astrophysics

Charge Fluids, Reissner-Nordstrom, General Relativity, Exact Solution

Scientific paper

In the present article models of well behaved charged superdense stars with surface density 2×1014 gm/cm3 are constructed by considering a static spherically symmetric metric with t = const hypersurfaces as spheroids and hyperboloids. Maximum mass of the star is found to be 7.66300 M Θ with radius 19.35409 km for spheroids case while 1.51360 M Θ with radius 13.72109 km for hyperboloid case satisfying ultra-relativistic conditions. The solutions thus found satisfy all the reality and causality conditions. For brevity we don't present a detailed analysis of the derived solutions in this paper.

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