Suppose M is a compact two-dimensional orientable Riemannian manifold with boundary ∂M. Denote by K the Gaussian curvature at points of M, and by kg the geodesic curvature at points of ∂M. Then
The theorem applies in particular if the manifold does not have a boundary, in which case the integral ∫∂M kg ds can be omitted.
If one bends and deforms the manifold M, its Euler characteristic will not change, while the curvatures at given points will. The theorem requires, somewhat surprisingly, that the total integral of all curvatures will remain the same.
A generalisation to n dimensions was found in the 1940s, by Allendoerfer, Weil, and Chern.