Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2019/ii/paper-2/36d/a/solution

This is the Schwarzschild-de Sitter spacetime. Its geodesic Lagrangian may be taken as
Time-translation and rotational symmetry give three independent integrals of motion, which may be chosen as
The constant norm of the tangent is , where for a timelike geodesic parametrized by proper time and for a null geodesic. Substitution gives
and hence

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