Gromov–Hausdorff distance measures how far two compact metric spaces are from being isometric. If X and Y are two compact metric spaces, then dGH (X,Y ) is defined to be the infimum of all numbers dH(f (X ), g (Y )) for all metric spaces M and all isometric embeddings f :X→M and g :Y→M. Here dH denotes Hausdorff distance between subsets in M and the isometric embedding is understood in the global sense, i.e. it must preserve all distances, not only infinitesimally small ones; for example no compact Riemannian manifold of negative sectional curvature admits such an embedding into Euclidean space.
The Gromov–Hausdorff distance turns the set of all isometry classes of compact metric spaces into a metric space, called Gromov–Hausdorff space, and it therefore defines a notion of convergence for sequences of compact metric spaces, called Gromov–Hausdorff convergence. A metric space to which such a sequence converges is called the Hausdorff limit of the sequence.
Some properties of Gromov–Hausdorff space
Pointed Gromov–Hausdorff convergence
Pointed Gromov–Hausdorff convergence is an appropriate analog of Gromov–Hausdorff convergence for non-compact spaces.
Given a sequence (Xn, pn) of locally compact complete length metric spaces with distinguished points, it converges to (Y, p) if for any R > 0 the closed R-balls around pn in Xn converge to the closed R-ball around p in Y in the usual Gromov–Hausdorff sense.
The notion of Gromov–Hausdorff convergence was first used by Gromov to prove that any discrete group with polynomial growth is virtually nilpotent (i.e. it contains a nilpotent subgroup of finite index). See Gromov's theorem on groups of polynomial growth. (Also see D. Edwards for an earlier work.) The key ingredient in the proof was the observation that for the Cayley graph of a group with polynomial growth a sequence of rescalings converges in the pointed Gromov–Hausdorff sense.
Another simple and very useful result in Riemannian geometry is Gromov's compactness theorem, which states that the set of Riemannian manifolds with Ricci curvature ≥ c and diameter ≤ D is relatively compact in the Gromov–Hausdorff metric. The limit spaces are metric spaces. Additional properties on the length spaces have been proven by Cheeger and Colding.
The Gromov–Hausdorff distance metric has been applied in the field of computer graphics and computational geometry to find correspondences between different shapes.
The Gromov–Hausdorff distance has been used by Sormani to prove the stability of the Friedmann model in Cosmology. This model of cosmology is not stable with respect to smooth variations of the metric.
- D.Burago, Yu.Burago, S.Ivanov, A Course in Metric Geometry, AMS GSM 33, 2001 (readable by first year graduate students).
- A.Ivanov, N.Nikolaeva, A.Tuzhilin (2015), The Gromov-Hausdorff Metric on the Space of Compact Metric Spaces is Strictly Intrinsic, arXiv:1504.03830
- Cheeger-Colding: On the structure of spaces with Ricci curvature bounded below I
- Sormani: Friedmann cosmology and almost isotropy
- Kotani M., Sunada T., Large deviation and the tangent cone at infinity of a crystal lattice, Math. Z. 254, (2006), 837-870.
- D. Edwards, "The Structure of Superspace", in "Studies in Topology", Academic Press, 1975, pdf
- M. Gromov. "Structures métriques pour les variétés riemanniennes", edited by Lafontaine and Pierre Pansu, 1980.
- M. Gromov. Metric structures for Riemannian and non-Riemannian spaces, Birkhäuser (1999). ISBN 0-8176-3898-9 (translation with additional content).