In closed universes with time-varying dark energy, deceleration-to-acceleration transition and dark energy domination start later than in flat cases, with stronger inflation-era acceleration and later deceleration; the reverse holds for open universes.
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The Effects of Spatial Curvature on Cosmic Evolution
In closed universes with time-varying dark energy, deceleration-to-acceleration transition and dark energy domination start later than in flat cases, with stronger inflation-era acceleration and later deceleration; the reverse holds for open universes.