Intuitively speaking, the exponential map takes a given tangent vector to the manifold, runs along the geodesic starting at that point and goes in that direction, for one unit of time. Since
v corresponds to the velocity vector of the geodesic, the actual (Riemannian) distance traveled will be dependent on that. We can also reparametrize geodesics to be unit speed, so equivalently we can define exp
p(
v) = β(|
v|) where β is the unit-speed geodesic (geodesic parameterized by arc length) going in the direction of
v. As we vary the tangent vector
v we will get, when applying exp
p, different points on
M which are within some distance from the base point
p—this is perhaps one of the most concrete ways of demonstrating that the tangent space to a manifold is a kind of "linearization" of the manifold. The
Hopf–Rinow theorem asserts that it is possible to define the exponential map on the whole tangent space if and only if the manifold is complete as a
metric space (which justifies the usual term
geodesically complete for a manifold having an exponential map with this property). In particular,
compact manifolds are geodesically complete. However even if exp
p is defined on the whole tangent space, it will in general not be a global
diffeomorphism. However, its differential at the origin of the tangent space is the
identity map and so, by the
inverse function theorem we can find a neighborhood of the origin of T
pM on which the exponential map is an embedding (i.e., the exponential map is a local diffeomorphism). The radius of the largest ball about the origin in T
pM that can be mapped diffeomorphically via exp
p is called the
injectivity radius of
M at
p. The
cut locus of the exponential map is, roughly speaking, the set of all points where the exponential map fails to have a unique minimum. An important property of the exponential map is the following
lemma of Gauss (yet another
Gauss's lemma): given any tangent vector
v in the domain of definition of exp
p, and another vector
w based at the tip of
v (hence
w is actually in the
double-tangent space T
v(T
pM)) and orthogonal to
v,
w remains orthogonal to
v when pushed forward via the exponential map. This means, in particular, that the boundary sphere of a small ball about the origin in T
pM is orthogonal to the geodesics in
M determined by those vectors (i.e., the geodesics are
radial). This motivates the definition of
geodesic normal coordinates on a Riemannian manifold. The exponential map is also useful in relating the
abstract definition of curvature to the more concrete realization of it originally conceived by Riemann himself—the
sectional curvature is intuitively defined as the
Gaussian curvature of some surface (i.e., a slicing of the manifold by a 2-dimensional submanifold) through the point
p in consideration. Via the exponential map, it now can be precisely defined as the Gaussian curvature of a surface through
p determined by the image under exp
p of a 2-dimensional subspace of T
pM. == Relationships to exponential maps in Lie theory ==