Bianchi Type-I Cosmological Models with Variable G and 4Λ$-Terms in General Relativity
arXiv:0705.0459 · doi:10.1007/s10509-008-9742-6
Abstract
Einstein's field equations with variable gravitational and cosmological ``constant'' are considered in presence of perfect fluid for Bianchi type-I spacetime. Consequences of the four cases of the phenomenological decay of have been discussed which are consistent with observations. The physical significance of the cosmological models have also been discussed.
12 pages, no figure
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