Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2019/iii/paper-310/1/c/solution

Normalize the present scale factor to . In a flat universe containing radiation in cosmology, pressureless matter, and a cosmological constant, the Friedmann equation is
where . Since , the age of an FLRW universe is
For a matter-only flat Einstein-de Sitter universe,
Taking the present value , for which the Hubble time is , gives

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