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General Relativity: An Introduction for Physicists · Problem 3.16
Vector calculus on manifolds — Hobson, Efstathiou & Lasenby
Physics · geodesic-intrinsic-derivative-alternative-form
Problem If x μ ( λ ) x^\mu(\lambda) x μ ( λ ) is an affinely parameterised geodesic, show that
D u μ D λ = 0 , \frac{Du^\mu}{D\lambda} = 0, D λ D u μ = 0 ,
where u μ = d x μ / d λ u^\mu = dx^\mu/d\lambda u μ = d x μ / d λ . Hence show that the geodesic equations can be written as
d u μ d λ = 1 2 ( ∂ μ g ν σ ) u ν u σ . \frac{du_\mu}{d\lambda} = \frac{1}{2}(\partial_\mu g_{\nu\sigma})u^\nu u^\sigma. d λ d u μ = 2 1 ( ∂ μ g ν σ ) u ν u σ .
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