The Euclidean black hole has topology ℜ2×Sd−2. It is
shown that -in Einstein's theory- the deficit angle of a cusp at any point in
ℜ2 and the area of the Sd−2 are canonical conjugates. The
black hole entropy emerges as the Euler class of a small disk centered at the
horizon multiplied by the area of the Sd−2 there.These results are
obtained through dimensional continuation of the Gauss-Bonnet theorem. The
extension to the most general action yielding second order field equations for
the metric in any spacetime dimension is given.Comment: 7 pages, RevTe