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Bianchi Type-III Cosmological Models with Gravitational Constant G and the Cosmological Constant ∧ |
| J. P. Singh1;R. K. Tiwari2;Pratibha Shukla2 |
| 1Department of Mathematical Sciences, A.P.S. University, Rewa (MP), India2Department of Mathematics, Govt. Model Science College, Rewa (MP), India |
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| Cite this article: |
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J. P. Singh, R. K. Tiwari, Pratibha Shukla 2007 Chin. Phys. Lett. 24 3325-3327 |
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Abstract Einstein field equations with variable gravitational and cosmological constants are considered in the presence of perfect fluid for the Bianchi type-III universe by assuming conservation law for the energy-momentum tensor. Exact solutions of the field equations are obtained by using the scalar of expansion proportional to the shear scalar θ∝σ, which leads to a relation between metric potential B= Cn, where n is a constant. The corresponding physical interpretation of the cosmological solutions are also discussed.
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04.20.Jb
98.80.Cq
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Received: 22 August 2007
Published: 03 December 2007
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| PACS: |
04.20.Jb
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(Exact solutions)
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98.80.Cq
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(Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))
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