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The diagram shows the classification of the cosmological models with > 0 according to the values of the parameters 0 and M0

The diagram shows the classification of the cosmological models with Λ > 0 according to the values of the parameters Ω Λ0 and Ω M0 . A straight line could be added to this figure that would separate the models that are currently accelerating from those that are currently decelerating. Starting from the Friedmann equations, derive the equation of this line. Note: Do not involve the q 0 parameter.

no big bang 2 expands forever closed open recollapses 3 2.

Note: Do not involve the q 0 parameter.

no big bang 2 expands forever closed pen recollapses 2 3

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