Riemannian manifold
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In Riemannian geometry, a Riemannian manifold (M,g) (with Riemannian metric g) is a real differentiable manifold M in which each tangent space is equipped with an inner product g in a manner which varies smoothly from point to point. This allows one to define various notions such as angles, lengths of curves, areas (or volumes), curvature, gradients of functions and divergence of vector fields. In other words, a Riemannian manifold is a differentiable manifold in which the tangent space at each point is a finite-dimensional Hilbert space. The terms are named after German mathematician Bernhard Riemann.
OverviewThe tangent bundle of a smooth manifold M assigns to each fixed point of M a vector space called the tangent space, and each tangent space can be equipped with an inner product. If such a collection of inner products on the tangent bundle of a manifold varies smoothly as one traverses the manifold, then concepts that were defined only pointwise at each tangent space can be extended to yield analogous notions over finite regions of the manifold. For example, a smooth curve α(t): [0, 1] → M has tangent vector α′(t0) in the tangent space TM(t0) at any point t0 ∈ (0, 1), and each such vector has length ||α′(t0)||, where ||·|| denotes the norm induced by the inner product on TM(t0). The integral of these lengths gives the length of the curve α:
Every smooth submanifold of Rn has an induced Riemannian metric g: the inner product on each tangent space is the restriction of the inner product on Rn. In fact, as follows from the Nash embedding theorem, all Riemannian manifolds can be realized this way. In particular one could define Riemannian manifold as a metric space which is isometric to a smooth submanifold of Rn with the induced intrinsic metric, where isometry here is meant in the sense of preserving the length of curves. This definition might theoretically not be flexible enough, but it is quite useful to build the first geometric intuitions in Riemannian geometry. Riemannian manifolds as metric spacesUsually a Riemannian manifold is defined as a smooth manifold with a smooth section of the positive-definite quadratic forms on the tangent bundle. Then one has to work to show that it can be turned to a metric space: If γ: [a, b] → M is a continuously differentiable curve in the Riemannian manifold M, then we define its length L(γ) in analogy with the example above by
Even though Riemannian manifolds are usually "curved", there is still a notion of "straight line" on them: the geodesics. These are curves which locally join their points along shortest paths. Assuming the manifold is compact, any two points x and y can be connected with a geodesic whose length is d(x,y). Without compactness, this need not be true. For example, in the punctured plane R2 \ {0}, the distance between the points (−1, 0) and (1, 0) is 2, but there is no geodesic realizing this distance. PropertiesIn Riemannian manifolds, the notions of geodesic completeness, topological completeness and metric completeness are the same: that each implies the other is the content of the Hopf-Rinow theorem. Riemannian metricsLet M be a second countable Hausdorff differentiable manifold of dimension n. A Riemannian metric on M is a family of inner products
be a basis of tangent vectors over Failed to parse (Missing texvc executable; please see math/README to configure.): p\in M . Then, the coefficients
is a Riemannian manifold. Examples
identified with Failed to parse (Missing texvc executable; please see math/README to configure.): e_i=(0,\dots, 1,\dots, 0) , the standard metric over an open subset Failed to parse (Missing texvc executable; please see math/README to configure.): U\subset\mathbb R^n is defined by
be a submanifold of M. Then the restriction of g to vectors tangent along N defines a Riemannian metric over N.
. The metric induced from Failed to parse (Missing texvc executable; please see math/README to configure.): \mathbb R^n
on Failed to parse (Missing texvc executable; please see math/README to configure.): S^{n-1}
is called the canonical metric of Failed to parse (Missing texvc executable; please see math/README to configure.): S^{n-1}
.
and Failed to parse (Missing texvc executable; please see math/README to configure.): M_2 be two Riemannian manifolds and consider the cartesian product Failed to parse (Missing texvc executable; please see math/README to configure.): M_1\times M_2 with the product structure. Furthermore, let Failed to parse (Missing texvc executable; please see math/README to configure.): \pi_1:M_1\times M_2\rightarrow M_1 and Failed to parse (Missing texvc executable; please see math/README to configure.): \pi_2:M_1\times M_2\rightarrow M_2 be the natural projections. For Failed to parse (Missing texvc executable; please see math/README to configure.): (p,q)\in M_1\times M_2 , a Riemannian metric on Failed to parse (Missing texvc executable; please see math/README to configure.): M_1\times M_2 can be introduced as follows :
possesses for example a Riemannian structure obtained by choosing the induced Riemannian metric from Failed to parse (Missing texvc executable; please see math/README to configure.): \mathbb R^2 on the circle Failed to parse (Missing texvc executable; please see math/README to configure.): S^1\subset \mathbb R^2 and then taking the product metric. The torus Failed to parse (Missing texvc executable; please see math/README to configure.): T^n endowed with this metric is called the flat torus.
be two metrics on Failed to parse (Missing texvc executable; please see math/README to configure.): M . Then,
The pullback metricIf f:M→N is a diffeomorphism and (N,gN) be a Riemannian manifold, then the pullback of gN along f is a Riemannian metric on M. The pullback is the metric f*gN on M defined for v, w ∈ TpM by
Existence of a metricEvery paracompact differentiable manifold admits a Riemannian metric. To prove this result, let M be a manifold and {(Uα, φ(Uα))|α∈I} a locally finite atlas of open subsets U of M and diffeomorphisms onto open subsets of Rn
IsometriesLet Failed to parse (Missing texvc executable; please see math/README to configure.): (M, g^M) and Failed to parse (Missing texvc executable; please see math/README to configure.): (N, g^N) be two Riemannian manifolds, and Failed to parse (Missing texvc executable; please see math/README to configure.): f:M\rightarrow N be a diffeomorphism. Then, f is called an isometry, if
is called a local isometry at Failed to parse (Missing texvc executable; please see math/README to configure.): p\in M if there is a neighbourhood Failed to parse (Missing texvc executable; please see math/README to configure.): U\subset M , Failed to parse (Missing texvc executable; please see math/README to configure.): U\ni p , such that Failed to parse (Missing texvc executable; please see math/README to configure.): f:U\rightarrow f(U) is a diffeomorphism satisfying the previous relation. Riemannian manifolds as metric spacesA connected Riemannian manifold carries the structure of a metric space whose distance function is the arclength of a minimizing geodesic. Specifically, let (M,g) be a connected Riemannian manifold. Let Failed to parse (Missing texvc executable; please see math/README to configure.): c:[a,b]\rightarrow M be a parametrized curve in M, which is differentiable with velocity vector c′. The length of c is defined as
can be parametrized by its arc length. A curve is parametrized by arclength if and only if Failed to parse (Missing texvc executable; please see math/README to configure.): \|c'(t)\|=1 for all Failed to parse (Missing texvc executable; please see math/README to configure.): t\in[a,b] . The distance function d : M×M → [0,∞) is defined by
where the infimum extends over all differentiable curves γ beginning at p∈M and ending at q∈M. This function d satisfies the properties of a distance function for a metric space. The only property which is not completely straightforward is to show that d(p,q)=0 implies that p=q. For this property, one can use a normal coordinate system, which also allows one to show that the topology induced by d is the same as the original topology on M. DiameterThe diameter of a Riemannian manifold M is defined by
Geodesic completenessA Riemannian manifold M' is geodesically complete if for all Failed to parse (Missing texvc executable; please see math/README to configure.): p\in M , the exponential map Failed to parse (Missing texvc executable; please see math/README to configure.): \exp_p is defined for all Failed to parse (Missing texvc executable; please see math/README to configure.): v\in T_pM , i.e. if any geodesic Failed to parse (Missing texvc executable; please see math/README to configure.): \gamma(t) starting from p is defined for all values of the parameter Failed to parse (Missing texvc executable; please see math/README to configure.): t\in\mathbb R . The Hopf-Rinow theorem asserts that M is geodesically complete if and only if it is complete as a metric space. If M is complete, then M is non-extentable in the sense that it is not isometric to a proper submanifold of any other Riemannian manifold. The converse is not true, however: there exist non-extendable manifolds which are not complete. See also
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References
es:Variedad de Riemann fr:Variété riemannienne it:Varietà riemanniana he:מטריקה רימנית nl:Riemann-variëteit fi:Riemannin monisto sv:Riemannmångfald |


