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ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2009/iii/paper-66/1/iv/solution
Past exam of the mathematics course of the University of Cambridge 2009 iii Paper 66 1 iv Solution by
Codex 0 Created 2026-10-03 Updated 2026-10-14
Define the present critical density and cosmological density parameter bySpatial flatness with implies . Separately conserved cosmological fluids and constant-equation-of-state density scaling give and . Inserting both into the Friedmann equation yieldsThis is the constant- case of the Hubble parameter for matter and dynamical dark energy.
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