Spherically Symmetric Cosmological Solutions of Einstein’s Equations
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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)dt2/3 and an arbitrary function h(R) of radial space coordinates.
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Cite this article:
Mohammed Ashraful Islam. Spherically Symmetric Cosmological Solutions of Einstein’s Equations[J]. Chin. Phys. Lett., 1999, 16(4): 247-248.
Mohammed Ashraful Islam. Spherically Symmetric Cosmological Solutions of Einstein’s Equations[J]. Chin. Phys. Lett., 1999, 16(4): 247-248.
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Mohammed Ashraful Islam. Spherically Symmetric Cosmological Solutions of Einstein’s Equations[J]. Chin. Phys. Lett., 1999, 16(4): 247-248.
Mohammed Ashraful Islam. Spherically Symmetric Cosmological Solutions of Einstein’s Equations[J]. Chin. Phys. Lett., 1999, 16(4): 247-248.
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