Solution

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

Write for the Hubble parameter. Subtracting the Friedmann equation from the second equation gives the Friedmann acceleration equation,
Since , eliminating with the first equation yields
Differentiating the first equation, with constant cosmological constant and curvature parameter, now gives
Thus the cosmological perfect-fluid continuity equation is . Multiplying by and using proves
This is local conservation of energy: expansion changes the energy in a comoving volume through pressure work.

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