A class of well behaved charged analogues of Vaidya-Tikekar type super-dense star

Details A class of well behaved charged analogues of Vaidya-Tikekar type super-dense star A class of well behaved charged analogues of Vaidya-Tikekar type super-dense star

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.334..273g&link_type=abstract

Astrophysics and Space Science, Volume 334, Issue 2, pp.273-279

Astronomy and Astrophysics

Astrophysics

2

Exact Solutions, Charged Fluids, Superdense Stars, General Relativity

Scientific paper

In the present article a model of well behaved charged superdense star with surface density 2×1014 gm/cm3 is constructed by considering a static spherically symmetric metric with t=const hypersurfaces as hyperboloid. So far well behaved model described by such metric could not be obtained. Maximum mass of the star is found to be 0.343457 M &sun; and the corresponding radius is 9.57459 km. The red shift at the centre and on the surface are given as 0.068887 and 0.031726 respectively.

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