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Complete Riemannian Metric


The geodesics in a complete Riemannian metric go on indefinitely, i.e., each geodesic is isometric to the real line. For example, Euclidean space is complete, but the open unit disk is not complete since any geodesic ends at a finite distance. Whether or not a manifold is complete depends on the metric.

CompleteRiemannianHole

For instance, the punctured plane R^2-(0,0) is not complete with the usual metric. However, with the Riemannian Metric ds^2=r^(-2)(dx^2+dy^2), the punctured plane is the infinite (flat) cylinder, which is complete. The figure above illustrates a geodesic which can only go a finite distance because it reaches a hole in the punctured plane, exemplifying that the punctured plane with the usual metric is not complete. The path (e^(T),0) is a geodesic parametrized by arc length.

Any metric on a compact manifold is complete. Consequently, the pullback metric on the universal cover of a compact manifold is complete.


See also

Compact Manifold, Geodesic, Hyperbolic Metric, Manifold, Riemannian Manifold, Riemannian Metric, Poincare Metric

This entry contributed by Todd Rowland

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Cite this as:

Rowland, Todd. "Complete Riemannian Metric." From MathWorld--A Wolfram Web Resource, created by Eric W. Weisstein. https://mathworld.wolfram.com/CompleteRiemannianMetric.html

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