Riemannian Geometry

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Riemannian geometry is the study of Riemannian manifolds, smooth manifolds that are equipped with a positive definite symmetric rank (2,0) tensor field g, called the metric.

Riemannian Distance

We can turn a Riemannian manifold into a metric space by defining the distance between points p and q to be

LaTeX: 
\min_\gamma \int_\gamma ds = \int_0^1 \sqrt{g(\gamma'(t),\gamma'(t))} dt,

where LaTeX: \gamma:(0,1) \to M is a curve connecting p and q.

To see that this coincides in the Euclidean case, assume first we have two points p and q in LaTeX: R^n that lie along the LaTeX: x^1 axis. Then for any curve LaTeX: \gamma = (\gamma^i) connecting them, we have

LaTeX: 
\int_0^1 \sqrt{g(\gamma'(t), \gamma'(t))} dt = \int_0^1 \sqrt{\sum_i {\gamma^i}'(t)^2} dt \ge \int_0^1 |{\gamma^i}'(t)| dt \ge \int_0^1 {\gamma^i}'(t) dt = \gamma(1) - \gamma(0) = q - p.

Suppose now that p and q are arbitrary points in LaTeX: R^n. We can find an element A of the Euclidean group mapping p and q to the LaTeX: x^1 axis. Since A preserves the metric, for any curve LaTeX: \gamma connecting p and q we have that

LaTeX: 
\int_0^1 \sqrt{g(\gamma'(t), \gamma'(t))} dt = \int_0^1 \sqrt{g(A_* \gamma'(t), A_* \gamma'(t))} dt = \int_0^1 \sqrt{g((A\circ\gamma)'(t), (A\circ\gamma)'(t))} dt.

Since LaTeX: A \circ \gamma is a curve connecting two points on the LaTeX: x^1 axis, we know that the smallest value of the above integral is the Euclidean distance between them, which is the Euclidean distance between p and q.

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