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Physics, 20.11.2020 17:10 aesthetickait

Consider a spatially flat, matter-dominated Universe (Ωm = Ω = 1), which is contracting with time. How does the density perturbation, δ ≡ (rho − rho¯)/rho¯, evolve with time in such a Universe? Here rho is the (average) density?

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Consider a spatially flat, matter-dominated Universe (Ωm = Ω = 1), which is contracting with time. H...
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