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I show that the de Sitter Equilibrium cosmology generically predictsobservable levels of curvature in the Universe today. The predicted value ofthe curvature depends only on the ratio of the density of non-relativisticmatter to energy density in cosmological constant, and the value of thecurvature from the initial bubble that starts the inflation. The result isindependent of the scale of inflation, the shape of the potential duringinflation, and many other details of the cosmology. Future cosmologicalmeasurements of the matter density, cosmological constant and curvature willopen up a window on the very beginning of our Universe and offer an opportunityto support or falsify the de Sitter Equilibrium cosmology.

Cosmic curvature from de Sitter equilibrium cosmology