Cosmological models with bulk viscosity in presence of adiabatic matter creation and with G, c and Lambda variables
arXiv:gr-qc/9812049 · doi:10.1023/A:1001930017624
Abstract
Some properties of cosmological models with a time variable bulk viscous coefficient in presence of adiabatic mater creation and G, c, Lambda variables are investigated in the framework of flat FRW line element. We trivially find a set of solutions through Dimensional Analysis. In all the studied cases it is found that the behaviour of these constants is inversely prportional to the cosmic time.
12 pages. We have been rewriting and completing the bibliography of this paper. Submitted to General Relativity and Gravitation
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