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Geodesic curvature : ウィキペディア英語版
Geodesic curvature
In Riemannian geometry, the geodesic curvature k_g of a curve \gamma measures how far the curve is from being a geodesic. In a given manifold \bar, the geodesic curvature is just the usual curvature of \gamma (see below), but when \gamma is restricted to lie on a submanifold M of \bar (e.g. for curves on surfaces), geodesic curvature refers to the curvature of \gamma in M and it is different in general from the curvature of \gamma in the ambient manifold \bar. The (ambient) curvature k of \gamma depends on two factors: the curvature of the submanifold M in the direction of \gamma (the normal curvature k_n), which depends only from the direction of the curve, and the curvature of \gamma seen in M (the geodesic curvature k_g), which is a second order quantity. The relation between these is k = \sqrt. In particular geodesics on M have zero geodesic curvature (they are "straight"), so that k=k_n, which explains why they appear to be curved in ambient space whenever the submanifold is.
==Definition==
Consider a curve \gamma in a manifold \bar, parametrized by arclength, with unit tangent vector T=d\gamma/ds. Its curvature is the norm of the covariant derivative of T: k = \|DT/ds \|. If \gamma 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 \mathbb^n, then the covariant derivative DT/ds is just the usual derivative dT/ds.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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