The universe experienced a transition from deceleration to acceleration approximately 5 billion years ago, as indicated by cosmological estimates. This shift is attributed to the dominance of dark energy over dark matter and baryons. In an expanding universe, the density of dark matter decreases more rapidly than that of dark energy, leading to this acceleration. Specifically, when the universe's volume doubles, dark matter density is halved while dark energy density remains constant. Understanding this transition is crucial for cosmological models and theories regarding the universe's expansion.