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Parallel transport, Christoffel symbols and the geodesic equation

Parallel transport compares vectors along a specified path. For the Levi-Civita connection, Christoffel symbols come from the metric and correct component derivatives. With an affine parameter, a geodesic parallel-transports its tangent; spacetime free fall follows a timelike geodesic.

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What a learner can do afterwards

  • Computes Christoffel symbols from a simple metric
  • Explains why differentiating a vector field needs a correction term in curved coordinates
  • Writes the geodesic equation and identifies free fall as its solution

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To compare vectors at different points, choose a path and parallel-transport one vector along it. Different paths can give different comparisons. We use the Levi-Civita connection: it preserves the metric and has zero torsion. These conditions let the metric determine the transport rule. Partial derivatives of metric components measure their local rate of change in one coordinate while the other coordinates stay fixed.

For the Levi-Civita connection, Γⁱⱼₖ=(1/2)gⁱˡ(∂ⱼgₗₖ+∂ₖgₗⱼ−∂ₗgⱼₖ). Repeated indices are summed. In plain-text indices, ^ marks upper and _ marks lower; braces group indices. ∂_r means differentiation in r. In coordinates (r,θ), g=diag(1,r²) gives Γ^r_{θθ}=−(1/2)∂_r g_{θθ}=−r, since ∂_r(r²)=2r. Also Γ^θ_{rθ}=Γ^θ_{θr}=1/r. All other polar components vanish.

The vector derivative is ∇ⱼVⁱ=∂ⱼVⁱ+ΓⁱⱼₖVᵏ. The added term accounts for basis changes. In polar coordinates, ∇_θ V^r=∂_θ V^r−r V^θ. Here V^θ is an upper-index component, not V_θ. For r=3, V^θ=1 and ∂_θ V^r=0, this derivative is −3 even though the ordinary component derivative is zero.

Flat plane: polar metricr¨−r(θ˙)²=0θ¨+2r˙θ˙/r=0
Polar geodesic equations. Dots denote derivatives in affine parameter λ. If r and λ are dimensionless, the derivatives are dimensionless.

A path is xⁱ(λ), where λ labels points along it. dxⁱ/dλ gives tangent components; d²xⁱ/dλ² measures their rate of change. Dots in the polar equations mean λ derivatives. For an affine λ, the geodesic equation is d²xⁱ/dλ²+Γⁱⱼₖ(dxʲ/dλ)(dxᵏ/dλ)=0. The tangent's covariant derivative along the path is zero. In spacetime, an ideal test body with no nongravitational force follows a timelike geodesic; light follows a null geodesic.

Coordinate acceleration need not vanish on a geodesic. The Christoffel term can cancel it. Christoffel symbols can also be nonzero in flat space, as the polar example shows. A freely falling capsule has zero proper acceleration even when its coordinate position has a nonzero second derivative.

Test a proposed path by substituting it into the geodesic equation. For a circle with fixed r>0 and θ˙≠0, the polar radial equation becomes −r(θ˙)²=0, which fails. The circle's tangent changes covariantly. Its appearance on a coordinate drawing cannot replace this test.

Choose a transport path. The Levi-Civita symbols come from the metric and correct derivatives. With an affine parameter, a geodesic has a covariantly constant tangent.

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Parallel transport, Christoffel symbols and the geodesic equation · Science, ages 23 to 24 · LightMySky