Gromov's compactness theorem (geometry)

In the

Riemannian manifolds, the key assumption of his compactness theorem is automatically satisfied under an assumption on Ricci curvature. These theorems have been widely used in the fields of geometric group theory and Riemannian geometry

.

Metric compactness theorem

The

compact metric spaces which ensures that a subsequence converges to some metric space relative to the Gromov–Hausdorff distance:^[1]

Let $(X i, d i)$ be a sequence of compact metric spaces with uniformly bounded diameter. Suppose that for every positive number $ε$ there is a
metric balls
of radius $ε$ . Then the sequence $(X i, d i)$ has a subsequence which converges relative to the Gromov–Hausdorff distance.

The role of this theorem in the theory of Gromov–Hausdorff convergence may be considered as analogous to the role of the Arzelà–Ascoli theorem in the theory of uniform convergence.^[2] Gromov first formally introduced it in his 1981 resolution of the Milnor–Wolf conjecture in the field of geometric group theory, where he applied it to define the asymptotic cone of certain metric spaces.^[3] These techniques were later extended by Gromov and others, using the theory of ultrafilters.^[4]

Riemannian compactness theorem

Specializing to the setting of

geodesically complete Riemannian manifolds with a fixed lower bound on the Ricci curvature, the crucial covering condition in Gromov's metric compactness theorem is automatically satisfied as a corollary of the Bishop–Gromov volume comparison theorem. As such, it follows that:^[5]

Consider a sequence of closed Riemannian manifolds with a uniform lower bound on the Ricci curvature and a uniform upper bound on the diameter. Then there is a subsequence which converges relative to the Gromov–Hausdorff distance.

The limit of a convergent subsequence may be a metric space without any smooth or Riemannian structure.^[6] This special case of the metric compactness theorem is significant in the field of Riemannian geometry, as it isolates the purely metric consequences of lower Ricci curvature bounds.