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1, the spatial curvature today provides only a small, sub-dominant contribution to the total space-time curvature (see Eq. 40)). 82) being controlled by the parameter r t which is a monotonically increasing function of time in the standard cosmological model. 83) so that r t is increasing in both the matter-dominated ( = 2/3) and radiationdominated ( = 1/2) eras. This implies that the contribution of the spatial curvature becomes less and less significant as we go back in time, according to the standard-model equations.
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