Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2018/ii/paper-1/37e/c/solution

The Euler-Lagrange equation has the first integral
where the constant follows from the initial data. Combining this with proper-time normalization gives the Timelike geodesic in the expanding flat slicing of de Sitter spacetime:
Consequently
Integrating from , where , gives
As , the first ratio tends to , so
Thus tends to at the finite proper time .

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