Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2009/iii/paper-66/1/iv/solution

Define the present critical density and cosmological density parameter by
Spatial flatness with implies . Separately conserved cosmological fluids and constant-equation-of-state density scaling give and . Inserting both into the Friedmann equation yields
This is the constant- case of the Hubble parameter for matter and dynamical dark energy.

New to topics? Read the docs here!