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Zbl 0870.53073
Abdussattar; Vishwakarma, R.G.
Some FRW models with variable $G$ and $\Lambda$.
(English)
[J] Classical Quantum Gravity 14, No.4, 945-953 (1997). ISSN 0264-9381; ISSN 1361-6382/e

Summary: Einstein's field equations with $G$ and $\Lambda$ both varying with time are considered in the context of general homogeneous, isotropic universes in a way which conserves the energy momentum tensor of the matter content. It is found that the solutions of the field equations, which are based on the variation of $\Lambda$ as $R^{-2}$ but with different constants of proportionality, describe significantly different cosmological scenarios. It is also found that the non-static models with constant density having a vacuum-like equation of state are endowed with inflation for a wide class of functions $G(t)$ and $\Lambda (t)$, and a static universe with constant density without the vacuum-like equation of state can exist only for $k=1$ with constant $G$ and $\Lambda$.
MSC 2000:
*53Z05 Appl. of differential geometry to physics
83F05 Relativistic cosmology

Keywords: Einstein's equations; variable cosmological constant; variable gravitational constant

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