Λ-models revisited

Physics

Scientific paper

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Scientific paper

We solve the Einstein equations, considering a non-null cosmological constant, non-null tricurvature, a large variety of equations of state represented by p = αρ (α = const), for a perfect fluid and the Robertson-Walker metric. Though some of the formulae obtained were already identified as solutions of particular cases, it is the first time that the general case is being solved. We find also that the specific equation of state only matters for the early phase of the universe.

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