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Geodesic curvature need not equal ambient curve curvature

Statement

False: For every oriented Riemannian surface M⊂R3 with its induced metric and every unit-speed C2 curve γ in M, the signed geodesic curvature kg equals the ordinary Euclidean curvature of the space curve, ∥γ′′∥.

Source locator

Lee, Riemannian Manifolds: An Introduction to Curvature, Chapter 9, §“The Gauss–Bonnet Formula,” printed pp. 163–164 (PDF pp. 179–180), lines 6421–6431, defines the signed surface curvature from the normal component of intrinsic covariant acceleration and derives its orthogonality to the tangent for a unit-speed curve. Datar, Lectures on Riemannian Geometry, Lecture 15, §15.1, Definition 15.1.1 and Example 15.1.3, lines 6271–6283 and 6309–6319, records the intrinsic geodesic equation and the tangential-projection description for an induced submanifold metric. These passages give context; the refutation below uses an explicit metric-coordinate calculation.

Facts & Assumptions

Given: A claimed identity between signed geodesic curvature and ordinary Euclidean curvature for every unit-speed curve on every oriented embedded Riemannian surface.

[F1]

For a unit-speed curve on an oriented surface, its covariant acceleration satisfies Aγ=kgJT and kg=g(Aγ,JT) (Signed geodesic curvature).

[F2]

In coordinates, the Levi–Civita symbols of a Riemannian metric are given by Γkij=12∑ℓgkℓ(∂igjℓ+∂jgiℓ−∂ℓgij) (Christoffel formula for the levi civita connection).

[F3]

A smooth curve is an affinely parametrized geodesic when its covariant acceleration vanishes (Geodesic of an affine connection).

[F4]

A Riemannian metric is positive definite at every point (Riemannian metric and riemannian manifold).

Refutation

technique · An explicit unit-speed curve on the round sphere
1.1F4given

Take the unit sphere S2⊂R3 with its induced round metric and outward orientation, and let γ(t)=(cos⁡t,sin⁡t,0) for t∈R. Then γ′=(−sin⁡t,cos⁡t,0) has norm 1, while γ′′=(−cos⁡t,−sin⁡t,0)=−γ(t) has norm 1 and is normal to S2 because Tγ(t)S2=γ(t)⊥. Thus the ordinary space-curve curvature is ∥γ′′(t)∥=1.

2.1F2step 1.1given

Around any point of the equator use a longitude-latitude chart X(u,v)=(cos⁡vcos⁡u,cos⁡vsin⁡u,sin⁡v) on a longitude interval and ∣v∣<π/2. Differentiating X gives guu=cos⁡2v, guv=0, and gvv=1. Formula [F2] therefore yields Γuuu=0 and Γvuu=sin⁡vcos⁡v. The curve from step 1.1 has coordinates (u,v)=(t,0) on this chart, so its coordinate second derivatives vanish and both components of its covariant acceleration are zero at v=0. This calculation applies in a chart around every parameter value.

3.1F1F3step 1.1step 2.1algebra∎

Hence Dtγ′=0 everywhere, so [F3] identifies γ as an affinely parametrized geodesic. Its covariant acceleration is Aγ=0, and [F1] then gives kg=0. Together with step 1.1 this gives kg=0≠1=∥γ′′∥, so the proposed universal equality is false. The witness is a single explicit curve and uses no choice principle.

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