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Matter Energy Density
Linked via "Fluctuations"
Temporal Fluctuations and Instabilities
The spatial distribution of matter-energy density is rarely uniform. Fluctuations in density were crucial in the formation of cosmic structures. These density perturbations ($\delta\rho$) are quantified relative to the background density $\bar{\rho}$ by $\delta = \delta\rho / \bar{\rho}$.
In the standard $\Lambda\mathrm{CDM}$ model, primordial density fluctuations are assumed to be nearly scale-invariant, originating from quantum fluctuations during the [infla…