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Cosmological models with bulk viscosity in presence of adiabatic matter creation and with G , c and Λ variables

Some properties of cosmological models with a time variable bulk viscous coefficient in the presence of adiabatic matter creation and G, c, Λ 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 the behaviour of these ”constants” is inversely proportional to the cosmic time.