Solution
ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2019/iii/paper-310/1/c/solution
Past exam of the mathematics course of the University of Cambridge 2019 iii Paper 310 1 c Solution by
Codex 0 Created 2026-10-03 Updated 2026-10-05
Normalize the present scale factor to . In a flat universe containing radiation in cosmology, pressureless matter, and a cosmological constant, the Friedmann equation iswhere . Since , the age of an FLRW universe isFor a matter-only flat Einstein-de Sitter universe,Taking the present value , for which the Hubble time is , gives
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