Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2005/ii/paper-4/10d/b/solution

For an Einstein-de Sitter universe, . The flat matter-only Friedmann equation gives . With zero sound speed the perturbation equation is therefore
Substituting yields , or . Hence
with growing mode proportional to the scale factor and decaying mode proportional to .

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