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

被引：1

作者：

Y. K. Gupta

Jitendra Kumar

机构：

[1] Indian Institute of Technology Roorkee,Department of Mathematics

来源：

Astrophysics and Space Science | 2011年 / 334卷

关键词：

Exact solutions; Charged fluids; Superdense stars; General relativity;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

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 0.343457M⊙ 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.

引用

页码：273 / 279

页数：6

共 10 条

[1]

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[2]

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[8]

Ivanov B.V.(undefined)undefined undefined undefined undefined-undefined

[9]

Vaidya P.C.(undefined)undefined undefined undefined undefined-undefined

[10]

Tikekar R.(undefined)undefined undefined undefined undefined-undefined

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