Geodesic curvature

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In Riemannian geometry, the geodesic curvature kg of a curve γ measures how far the curve is from being a geodesic. For example, for 1D curves on a 2D surface embedded in 3D space, it is the curvature of the curve projected onto the surface's tangent plane. More generally, in a given manifold M¯, the geodesic curvature is just the usual curvature of γ (see below). However, when the curve γ is restricted to lie on a submanifold M of M¯ (e.g. for curves on surfaces), geodesic curvature refers to the curvature of γ in M and it is different in general from the curvature of γ in the ambient manifold M¯. The (ambient) curvature k of γ depends on two factors: the curvature of the submanifold M in the direction of γ (the normal curvature kn), which depends only on the direction of the curve, and the curvature of γ seen in M (the geodesic curvature kg), which is a second order quantity. The relation between these is k=kg2+kn2. In particular geodesics on M have zero geodesic curvature (they are "straight"), so that k=kn, which explains why they appear to be curved in ambient space whenever the submanifold is.

Definition

Consider a curve γ in a manifold M¯, parametrized by arclength, with unit tangent vector T=dγ/ds. Its curvature is the norm of the covariant derivative of T: k=DT/ds. If γ lies on M, the geodesic curvature is the norm of the projection of the covariant derivative DT/ds on the tangent space to the submanifold. Conversely the normal curvature is the norm of the projection of DT/ds on the normal bundle to the submanifold at the point considered.

If the ambient manifold is the euclidean space n, then the covariant derivative DT/ds is just the usual derivative dT/ds.

If γ is unit-speed, i.e. γ(s)=1, and N designates the unit normal field of M along γ, the geodesic curvature is given by

kg=γ(s)(N(γ(s))×γ(s))=[d2γ(s)ds2,N(γ(s)),dγ(s)ds],

where the square brackets denote the scalar triple product.

Example

Let M be the unit sphere S2 in three-dimensional Euclidean space. The normal curvature of S2 is identically 1, independently of the direction considered. Great circles have curvature k=1, so they have zero geodesic curvature, and are therefore geodesics. Smaller circles of radius r will have curvature 1/r and geodesic curvature kg=1r2r.

Some results involving geodesic curvature

  • The geodesic curvature is none other than the usual curvature of the curve when computed intrinsically in the submanifold M. It does not depend on the way the submanifold M sits in M¯.
  • Geodesics of M have zero geodesic curvature, which is equivalent to saying that DT/ds is orthogonal to the tangent space to M.
  • On the other hand the normal curvature depends strongly on how the submanifold lies in the ambient space, but marginally on the curve: kn only depends on the point on the submanifold and the direction T, but not on DT/ds.
  • In general Riemannian geometry, the derivative is computed using the Levi-Civita connection ¯ of the ambient manifold: DT/ds=¯TT. It splits into a tangent part and a normal part to the submanifold: ¯TT=TT+(¯TT). The tangent part is the usual derivative TT in M (it is a particular case of Gauss equation in the Gauss-Codazzi equations), while the normal part is II(T,T), where II denotes the second fundamental form.
  • The Gauss–Bonnet theorem.

See also

References