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Isometric Embedding


An isometric embedding of metric spaces is a map f:X->Y preserving all pairwise distances, so that d_Y(f(x),f(y))=d_X(x,y) for all x,y in X. Such a map is necessarily injective, and is an isometry onto its image.

For Riemannian manifolds, an isometric embedding instead means a differentiable embedding preserving the metric tensor. If f:(M,g)->(P,h), the defining condition is

 h_(f(x))(df_x(v),df_x(w))=g_x(v,w),

where v,w belong to the tangent space at x. It preserves curve length and hence the intrinsic distances within the image, but need not preserve ambient distances. For example, the inclusion of the unit circle into the plane preserves arc length, while the Euclidean distance between opposite image points is 2 rather than the intrinsic distance pi. The Nash-Kuiper theorem concerns this Riemannian meaning.


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References

Borrelli, V.; Jabrane, S.; Lazarus, F.; and Thibert, B. "Flat Tori in Three-Dimensional Space and Convex Integration." Proc. Nat. Acad. Sci. USA 109, 7218-7223, 2012. https://doi.org/10.1073/pnas.1118478109.Nash, J. "C^1 Isometric Imbeddings." Ann. Math. 60, 383-396, 1954. https://doi.org/10.2307/1969840.

Cite this as:

Weisstein, Eric W. "Isometric Embedding." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/IsometricEmbedding.html

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