Expansion of the universe is set at the correct rate for stability

Jan 20, 2024 7:59 AM
Feb 14, 2024 5:18 PM

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A homogeneous universe is called “flat” if it is balanced between eventual gravitational collapse and eternal expansion; in such a case its geometry would be precisely Euclidean and space would not be curved. The universe achieves such flatness when the actual mass density in the universe is very close to the critical mass density (the density required to halt the expansion of the universe)—that is, if the ratio between the actual and critical mass densities is close to one. In our universe, the ratio of these two quantities is ever so slightly less than one. As a result, our universe will keep on expanding without a gravitational recollapse, and space has hardly any overall curvature. That these values were so precisely balanced is surprising from the standpoint of standard big-bang theory, because, again, for this balance to arise, the universe would have needed to have very finely tuned initial conditions.