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Spherically Symmetric Cosmological Solutions of Einstein’s Equations |
Mohammed Ashraful Islam |
Department of Mathematics, and Research Centre for Mathematical and Physical Sciences, Chittagong University, Chittagong, Bangladesh |
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Cite this article: |
Mohammed Ashraful Islam 1999 Chin. Phys. Lett. 16 247-248 |
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Abstract Two sets of solution of the Einstein’s equations of general theory of relativity which is spherically-symmetric and nonstatic homogeneous isotropic universe for perfect fluid are obtained. The first solution is the Einstein de-Sitter type containing a scale factor ( √6πкGt + a)4/3 and an arbitrary function f (R) of radial space coordinates. The second solution is for stiff equation of state p = ρc2, which also has a scale factor [3 √8πaG∫t0ξ(t)dt]2/3 and an arbitrary function h(R) of radial space coordinates.
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Keywords:
04.20.Jb
98.80.Dr
95.30.Sf
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Published: 01 April 1999
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