Decaying Lambda cosmology, varying G and holography

Details Decaying Lambda cosmology, varying G and holography Decaying Lambda cosmology, varying G and holography

2004-05-28

arxiv.org/abs/gr-qc/0405141v3

Int.J.Mod.Phys.A20:2465-2469,2005

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Minor changes. A short version will appear in the Int. J. Mod. Phys. A (Proceedings of the Sixth Alexander Friedmann Internati

Scientific paper

10.1142/S0217751X0502478X

We discuss a class of uniform and isotropic, spatially flat, decaying Lambda cosmologies, in the realm of a model where the gravitation constant G is a function of the cosmological time. Besides the usual de Sitter solution, the models at late times are characterized by a constant ratio between the matter and total energy densities. One of them presents a coasting expansion where the matter density parameter is equal to 1/3, and the age of the universe satisfies Ht = 1. From considerations in line with the holographic conjecture, it is argued that, among the non-decelerating solutions, the coasting expansion is the only acceptable from a thermodynamic viewpoint, and that the time varying cosmological term must be proportional to the square of the Hubble parameter, a result earlier obtained using different arguments.

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