Difference between revisions of "User:Yakovenko/sandbox1"
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== Related geometric notions == | == Related geometric notions == | ||
There are many other geometric notions intimately related to connections. For more details refer to the respective EOM articles. | There are many other geometric notions intimately related to connections. For more details refer to the respective EOM articles. | ||
+ | * [[Holonomy]] group. For a given base point , the holonomy group is the set of all self-maps of the fiber, obtained as parallel transport along closed loops beginning and ending at a. For non-simply connected base B the holonomy group may be nontrivial even for (locally) flat connections. | ||
* [[Geodesic line]] (sometimes ''Geodesic curve'' or just ''geodesic''). A smooth curve on a Riemannian manifold, whose velocity vector is parallel to itself along the curve. Geodesics are locally shortest paths (provide the minimum of the arc length integral among all curves connecting two sufficiently close points on the geodesic). | * [[Geodesic line]] (sometimes ''Geodesic curve'' or just ''geodesic''). A smooth curve on a Riemannian manifold, whose velocity vector is parallel to itself along the curve. Geodesics are locally shortest paths (provide the minimum of the arc length integral among all curves connecting two sufficiently close points on the geodesic). | ||
* [[Geodesic curvature]], [[Sectional curvature]], [[Ricci curvature]], [[mean curvature]], [[principal curvature]]. Various combinations of components of the general metric curvature tensor. One has to distinguish between the ''intrinsic'' invariants which depend only on the metric (e.g., induced on an embedded submanifold of a Riemannian manifold) and ''extrinsic'', depending on the embedding itself. | * [[Geodesic curvature]], [[Sectional curvature]], [[Ricci curvature]], [[mean curvature]], [[principal curvature]]. Various combinations of components of the general metric curvature tensor. One has to distinguish between the ''intrinsic'' invariants which depend only on the metric (e.g., induced on an embedded submanifold of a Riemannian manifold) and ''extrinsic'', depending on the embedding itself. |
Revision as of 05:40, 28 May 2012
Connection
\def\G{\varGamma}
An infinitesimal structure on a (smooth) bundle which allows to define the parallel transport between fibres of the bundle.
Historical overview
Initially the notion of connection appeared in the works by Gregorio Ricci and Tullio Levi-Civita who constructed the infinitesimal parallel transport between tangent spaces of a Riemannian manifold. Later the construction was distilled from the Riemannian context by Éli Cartan who constructed connections on principal bundles (equipped by action of a Lie group) and introduced the notion of the connection form. Finally, Charles Ehresmann gave a general definition of connection via distribution of horizontal subspaces, which is the most general construction using only the smooth structure and local triviality of the bundle.
In practice when dealing with connections, one distinguishes several particular cases of bundles and several (interrelated) ways to describe the infinitesimal parallel transport.
- Connections on the vector bundles, defined by an operator of covariant derivation;
- Affine connections on manifolds, defined on the tangent (and cotangent) bundle to a smooth manifold;
- Connections on G-bundles equipped with fibrewise action of a Lie group G;
- Levi-Civita (metric) connections on Riemannian manifolds, defined on the tangent bundle and preserving the metric structure.
Ehresmann connection
Let \pi:E\to B be a smooth bundle with a generic fiber F. An Ehresmann connection is a "horizontal" subbundle \G\subset TE of the tangent bundle, complementary to the "vertical" subbundle \operatorname{Ker}\rd \pi. In other words, the tangent space T_xE at any point x\in E is split as a direct sum of the vertical subspace V_x=T_x F_x tangent to the fiber F_x=\pi^{-1}(\pi(x)) through x, and a complementary subspace \G_x\subset T_x; by definition of complementarity, \dim\G_x=\dim B, and the restriction \rd \pi(x)|_{\G_x}\to T_{\pi(x)}B is an isomorphism.
This splitting allows to define the parallel transport along any smooth curve \gamma:[0,1]\to B between the fibers F_0=\pi^{-1}(\gamma(0)) and F_1=\pi^{-1}(\gamma(1)) as follows. Consider the induced bundle \pi'=\gamma^*\pi over the new base B'=[0,1]: because of the triviality of the segment [0,1], this bundle is trivial, with the total space E'\simeq F\times [0,1], and the horizontal subbundle \G induces a horizontal subbundle \G'=\gamma^*\G on E'. But since the base is now one-dimensional, the distribution \G' is integrable and defines the foliation on E', everywhere transversal to the fibers. Under mild additional conditions[1] the leaf (integral trajectory of the integrable distribution \G') passing through the point x\in F_0=F\times\{0\}, crosses the fiber F_1=F\times\{1\} at a unique point \tau_0^1(x)\in F_1. By the general theorems from ordinary differential equations, the map \tau=\tau_0^1 is a diffeomorphism (smooth and invertible self-map) of F.
G-invariant connection
Assume that \pi:E\to B is a bundle with a Lie group G acting freely and transitively on the fibers (and hence on the total space), say, by the right multiplication, E\times G\to E, r:(x,g)\mapsto x\cdot g, \pi(x\cdot g)=\pi(x). Then is natural to consider the equivariant (G-invariant) connections for which the horizontal subspaces \G_x and \G_{x\cdot g} are related by the differential of the corresponding right shift \rd r(\cdot,g).
Such invariance means that for any smooth curve \gamma the corresponding parallel transport \tau_\gamma:F_0\to F_1 commutes with the action of G: \tau(x\cdot g)=\tau(x)\cdot g for any g\in G. In other words, it is sufficient to construct the parallel transport for only one point on the fiber.
Note also that for principal G-bundles the tangent spaces T_x F_b to the same fiber \pi^{-1}(b) are canonically isomorphic to each other and to the tangent space T_e G=\mathfrak g which is a Lie algebra of the group G. The isomorphism is defined by the differential of the map (G,e)\to (F,x), g\mapsto x\cdot g.
Affine connection
If the generic fiber F of a bundle \pi:E\to B is a (finite-dimensional) vector space isomorphic to \R^n, then it is natural to consider affine[2] connections. By definition, a connection is affine, if all the parallel transport operators are linear (invertible) maps between the corresponding fibers.
The linear structure on the generic fiber induces the structure of a module (over the ring C^\infty(B) of smooth functions on the base) on the space of sections \Gamma(E)=\{s:B\to E,\ \pi\circ s=\operatorname{id}_B\}: For any two sections s_1,s_2:B\to E and any smooth function f:B\to \R the sum s_1+s_2:B\to E and the products f\cdot s_i:B\to E are well-defined smooth sections of \pi,
(s_1+s_2)(b)=s_1(b)+s_2(b),\qquad (f\cdot s_i)(b)=f(b)\cdot s_i(b),\qquad s_i(b)\in F_b=\pi^{-1}(b),\ f(b)\in \R.
Connection 1-forms (Lie-algebra-valued and matrix-valued)
For each Ehresmann connection on the principal bundle the splitting of the tangent space T_x E=V_x\oplus \G_x into the vertical and horizontal subspaces defines the linear projection of T_x E into the vertical component V_x parallel to the horizontal component \G_x. This projection can be interpreted as \mathfrak g-valued[3] differential 1-form \boldsymbol\omega on TE, which is "identical" on the vertical subspaces (recall that each vertical subspace V_x can be identified with \mathfrak g) and invariant by the right action of G. The horizontal subspace \G_x by construction is the common null space defined by the Pfaffian equations \boldsymbol\omega=0.
If the principal bundle \pi is defined by local trivializations and the corresponding cocycle \{g_{\alpha\beta}:U_{\alpha\beta}\to G\}, this means that points from G\times U_\alpha are identified with points from G\times U_\beta over U_{\alpha\beta}=U_\alpha\cap U_\beta by the gauge transformation rule (v_\alpha,b)\simeq (v_\beta,b)\ \iff\ v_\alpha=g_{\alpha\beta}\cdot v_\beta,\ v_\beta=g_{\beta\alpha}\cdot v_\alpha.\tag{GT}
In the trivialization over U_\alpha (resp., over U_\beta) the connection is defined the tuple of \mathfrak g-valued forms \boldsymbol\omega_\alpha (resp., \boldsymbol\omega_\beta). To be self-consistent over the intersection U_{\alpha\beta}, one tuple should be transformed into the other by the gauge transformation: for any two sections s_\alpha and s_\beta=g_{\beta\alpha}\cdot s_\alpha over U_{\alpha\beta}, the linear operators \boldsymbol\omega_\alpha\circ \rd s_\alpha: T_b B\to \mathfrak g and \boldsymbol\omega_\beta\circ \rd s_\beta:T_b B\to\mathfrak g must coincide after computing the differentials[4].
For an Ehresmann connection on a vector bundle the tangent space to the linear fiber F\simeq\R^n is naturally identified with itself, thus in a local trivialization \R^n\times U_\alpha with the coordinates (v_1,\dots,v_n,b_1,\dots,b_m) the connection form can be associated with the tuple of 1-forms \omega_{i\alpha}=\rd v_i-\sum_{k=1}^m F_{ik\alpha}(v,b)\rd b_k, where m=\dim B, and i=1,\dots,n=\dim F. If the connection is affine (see above), then the dependence of the coefficients F_{ik\alpha}(v,b) on v must be linear. This allows to write the (vector) connection form \boldsymbol\omega_\alpha as \boldsymbol\omega_\alpha=\rd v_\alpha-\Omega_\alpha\cdot v_\alpha,\qquad\Omega_\alpha=\begin{pmatrix} \theta_{11,\alpha}&\cdots&\theta_{1n,\alpha}\\ \vdots &\ddots&\vdots\\ \theta_{n1,\alpha}&\cdots&\theta_{nn,\alpha}\end{pmatrix},\quad v=\begin{pmatrix} v_{1,\alpha}\\ \vdots \\ v_{n,\alpha}\end{pmatrix}, \quad \rd v_\alpha=\begin{pmatrix} \rd v_{1,\alpha}\\ \vdots \\ \rd v_{n,\alpha}\end{pmatrix}, with \theta_{jk,\alpha} being 1-forms on the base U_\alpha\subseteq B, v_\alpha=(v_{1,\alpha},\dots,v_{n,\alpha}) the coordinates on the fiber and \rd v_\alpha their respective differentials. The matrix 1-form \Omega_\alpha is called the connection matrix[5] in the given trivialization.
The coefficients of the 1-forms \theta_{jk} are called the Christoffel symbols: \theta_{jk}=\sum_i\Gamma_{jk}^i(b)\,\rd b_i,\tag{C} where (b_1,\dots,b_m) are local coordinates in an open set U=U_\alpha, and \theta_{jk} the 1-forms constituting the connection matrix form over U. The Christoffel symbols are smooth functions on the base of a vector bundle.
Passing from one trivialization to another (over U_\beta) means replacing the coordinate vector v_\alpha by the new coordinate vector v_\beta=M_{\beta\alpha}\cdot v_\alpha with M_{\alpha\beta}(\cdot)=M^{-1}_{\beta\alpha}(\cdot) being a smooth matrix-valued function (cocycle) on U_{\alpha\beta}. Applying this gauge transformation, we conclude by the Leibniz rule[6] that \rd v_\beta=\rd (M_{\beta\alpha}\cdot v_\alpha)=\rd M_{\beta\alpha}\cdot v_\alpha+M_{\beta\alpha}\cdot \rd v_\alpha=(\rd M_{\beta\alpha}+M_{\beta\alpha}\Omega_\alpha)\cdot M_{\alpha\beta}\cdot v_\beta, that is, \Omega_\beta=\rd M_{\beta\alpha}\cdot M_{\alpha\beta}+M_{\beta\alpha}\cdot\Omega_\alpha \cdot M_{\alpha\beta} \tag{GC} (note the mnemonic order of indices \alpha,\beta). The transformation law (GC), sometimes called the gauge transformation of the connection matrux form, involves the "matrix logarithmic derivative" term \rd M\cdot M^{-1} and hence the matrices \Omega_\alpha "do not form a tensor".
Example. Let \gamma:[0,1]\to B a smooth path, t\mapsto \gamma(t), entirely belonging to one chart U=U_\alpha, with the corresponding matrix connection form \Omega=\Omega_\alpha. Then the induced connection on \R^n\times[0,1] is defined by system of linear ordinary differential equations with variable coefficients of the form \frac{\rd v}{\rd t}=A(t)\cdot v,\qquad A(t)=i_{\dot\gamma(t)}\,\Omega(\gamma(t)),\tag{LS} with the matrix of coefficients A obtained by evaluation of the matrix 1-form \Omega on the velocity vector \dot\gamma(t). The result of the parallel transport along \gamma is the value at t=1 of the fundamental matrix solution V(t) to the system (LS) with the initial condition V(0)=\operatorname{id}.
Covariant derivative
Any smooth section s\in\Gamma(E) of a vector bundle \pi:E\to B equipped with an affine connection, can be differentiated along any smooth curve \gamma:(\R^1,0)\to (B,b) in the base. By definition, the result, called the "absolute", or covariant derivative at the initial moment t=0, i.e., at the point b=\gamma(0), is the limit D_\gamma s(b)=\lim_{t\to 0}\tfrac1t(\tau_t^0 \bigl(s(t)\bigr)-s(0))\in \pi^{-1}(b), where \tau_t^0=(\tau_0^t)^{-1}:\pi^{-1}\bigl(\gamma(t)\bigr)\to\pi^{-1}\bigl(\gamma(0)\bigr) is the parallel transport between two close fibers over the points \gamma(t) and \gamma(0) on the curve.
From this definition and the linearity of \tau it follows that D_\gamma is the additive operation satisfying the Leibniz rule, if we extend it to smooth functions by the natural way as the Lie derivation[7]: D_\gamma(s_1+s_2)=D_\gamma s_1+D_\gamma s_2,\qquad D_\gamma (f\cdot s)=(D_\gamma f)\cdot s+f\cdot D_\gamma s.
In each trivializing chart U_\alpha a smooth section s(\cdot) can be identified with a vector-function s_\alpha:U_\alpha\to\R^n and the covariant derivative can be expressed through the matrix 1-form of the connection \Omega_\alpha as follows: D_\gamma s(b)=i_{\dot \gamma(0)}\bigl(\rd s_\alpha-\Omega_\alpha\cdot s_\alpha\bigr)=\left.\frac{\rd s_\alpha(\gamma(t))}{\rd t}\right|_{t=0}-A(b)\cdot s_\alpha(b),\qquad A(b)=(i_{\dot\gamma(0)}\Omega_\alpha)(b). This computation shows that the covariant derivative in fact depends only on the velocity vector w=\dot\gamma(0) of the curve \gamma, and does this in a linear way. Thus the covariant derive becomes a differential operator (usually denoted by \nabla_w) which generalizes the directional derivative \nabla_w f=i_w\rd f=L_w f: \nabla_w:\Gamma(E)\to\Gamma(E),\quad \forall f\in C^\infty(B),\qquad \nabla_{fw}=f\nabla_w,\quad \nabla_w(fs)=f\,(\nabla_w s)+(\nabla_w f)\, s.
Covariant derivative and the Christoffel symbols
To describe completely a linear connection in any trivializing chart F\times U\simeq \{(v,b):v=(v_1,\dots,v_n)\in\R^n,\ b=(b_1,\dots,b_m)\in V\subseteq\R^m\}, it is sufficient to specify the coefficients of the expansion of the covariant derivatives along all coordinate axes of n linear independent sections \mathrm e_1,\dots\mathrm e_n\in\Gamma(E), e.g., the coefficients \Gamma_{ij}^k=\Gamma_{ij}^k(b) of the expansions \nabla_{\frac\partial{\partial b_i}}\mathrm e_j=\sum_{k=1}^n\Gamma_{ij}^k(b)\mathrm e_k,\qquad\text{where}\quad\mathrm e_j(b)=(0,\dots,\underset{j}1,\dots,0),\quad j,k=1,\dots,n, \ i=1,\dots,m. These coefficients are the same Christoffel symbols (C).
Covariant derivative and parallel transport
A section s\in\Gamma(E) is said to be parallel along \gamma, if D_\gamma s\equiv0. If s is such a section, it defines the result of the parallel transport of the vector s(\gamma(0))\in F_{\gamma(0)} to be the vector s(\gamma(t))\in F_{\gamma(t)} for all points \gamma(t) on the curve.
For any vector v\in F_{a} and any curve \gamma:(\R^1,0)\to (B,a) one can construct a unique section s defined along \gamma and parallel along it with the initial condition s(a)=v. This section is constructed as a solution to a system of linear ordinary differential equations \frac{\rd }{\rd t}s(\gamma(t))=i_{\dot\gamma(t)}\Omega_\alpha(\gamma(t))\cdot s(\gamma(t)),\qquad s:(\R^1,0)\to\R^n in any trivializing chart.
Parallel transport is independent of the parametrization of the curve
If s is a section parallel along a curve \gamma, then this fact is not changed by another choice of the parametrization of \gamma. Indeed, this choice would replace the derivative D_\gamma by a (non-constant) multiple, without changing solutions of the equation D s=0.
Dual of the covariant derivative
The construction of the covariant derivative via the parallel transport allows to derivate also sections of the dual bundle. For a parametrized curve \gamma:(\R^1,0)\to (B,b) he family of linear operators \{\tau_t^s:F_t\to F_s,\ t,s\in(\R^1,0)\} defines the parallel translation between fibers F_t=\pi^{-1}(t) and F_s=\pi^{-1}(s) along \gamma. The dual bundle has fibers F_t^* dual to F_t, and the parallel transport is realized by the adjoint operators (\tau_t^s)^*={\tau^*}_s^t in the opposite direction. However, this allows to define the covariant directional derivative of sections of the dual bundle E^* using the same construction. If s\in\Gamma(E) and s^*\in\Gamma(E^*) are two sections of the dual bundles, then the parallel transport agrees with the pairing: \nabla_w\left< s, s^* \right>=\left< \nabla_w s,s^* \right> +\left< s,\nabla^*_w s^*\right> (the left hand side is the Lie derivative of the scalar function). This identity can be used to define the covariant derivative \nabla^*_w of the section s^* and the corresponding 1-form \nabla^*. If in a trivializing chart U_\alpha the covariant derivation takes the form \nabla=\rd -\Omega_\alpha, then \nabla^*=\rd +\Omega_\alpha^*, where \Omega^*_\alpha is the transpose (in the real case) of the matrix 1-form \Omega_\alpha.
In practice, however, the dual covariant derivative \nabla^* is denoted by the same symbol \nabla.
Covariant derivation of tensor and exterior products
The calculus of covariant derivations on a vector bundle E and its dual E^* extends naturally on bundles which fiberwise are tensor or exterior products of E and E^*. The corresponding formulas always have the form of suitable Leibniz identities, e.g., for a section s_1\otimes s_2 of the tensor product bundle E\otimes E its covariant derivative is computed as follows, \nabla(s_1\otimes s_2)=(\nabla s_1)\otimes s_2+s_1\otimes(\nabla s_2). Derivative of a wedge product of two sections \xi_1\land\xi_2 of the bundle E^*\land E^* follows the rule \nabla(\xi_1\land \xi_2)=(\nabla \xi_1)\land \xi_2+(-1)^n\xi_1\land (\nabla \xi_2),\qquad n=\dim F, etc. An important case is the maximal exterior power \bigwedge ^n E of the n-dimensional vector bundle E, a line (1-dimensional) bundle called the determinant bundle. By Liouville--Ostrogradskii formula, the corresponding covariant derivative is the trace \operatorname{tr}\nabla of the connection \nabla. In a trivializing chart in which \nabla=\rd-\Omega_\alpha, the trace takes the form \operatorname{tr}\nabla=\rd-\operatorname{tr}\Omega_\alpha, where the trace of a matrix 1-form \Omega_\alpha is the sum of (scalar) diagonal 1-forms.
Curvature of an affine connection
The main article is Curvature form.
The parallel transport between two different fibers of a vector bundle depends on the smooth (or piecewise-smooth) path connecting the base points. The curvature is a local differential expression of this dependence. More specifically, the curvature is a map which associates with any two vectors u_a,w_a\in T_a B tangent to the base, the properly normalized linear operator of parallel transport along the perimeter of an infinitesimally small parallelogram, a closed path in the base, with sides parallel to u_a and w_a. More precisely, let u,w be two commuting vector fields on B which extend the vectors u_a=u(a) and w_a=w(a). Then the curvature is the commutator of two differential operators[8],
R_{u,w}=\nabla_u\nabla_w-\nabla_w\nabla_u:\Gamma(E)\to\Gamma(E).
One can instantly verify that R_{\varphi u,\psi w}=\varphi\psi R_{u,w} and is additive in each argument u,w separately, thus R depends in the bilinear (antisymmetric) way on the vectors defining the "infinitesimally small loop".
A connection is called flat, if its curvature is zero, that is, the result of the parallel transport between two fibers does not depend on (small) variations of the path connecting the respective base points. The flatness is equivalent to vanishing of the curvature and commutation of the covariant derivatives along commuting vector fields. However, flat connections may have nontrivial parallel transport along non-contractible loops.
Connections on tangent/cotangent bundles of a smooth manifold
A very important particular case of linear connections are connections on the tangent bundle TM, which by duality descend on the cotangent bundle T^*M and their tensor/wedge products. For those connections one can compare the covariant derivatives \nabla_ w u and \nabla_u w for two vector fields u,w\in\Gamma(TM), sections of the same tangent bundle. This allows to introduce a subclass of linear connections, called symmetric connections.
A connection \nabla is symmetric, if for any two vector fields u,w \nabla_w u-\nabla_u w-[w,u]=0,\tag{T} with the commutator of two vector fields appearing in the right hand side.
Torsion tensor
The left hand side of the expression (T) depends on two vector fields u,w, but is a tensor field, not a derivation: if we replace these fields by \varphi u and \psi w, with \varphi,\psi being two (scalar) smooth functions, the result will be multiplied by the product \varphi\psi: \nabla_{\psi w}u-\nabla_u (\psi w)-[\psi w,u]=\psi\,\nabla_w u-(\nabla_u\psi)\, w-\psi\,\nabla_u w +(L_u \psi)w-\psi\,[w,u]=\psi\,(\nabla_w u-\nabla_u w-[w,u]), where L_u\psi=\nabla_u \psi=i_u\rd \psi is the Lie derivative of \psi along u, and the same regarding \varphi.
This is called the torsion tensor of the connection \nabla. Its vanishing means that the "second covariant derivative" in two different directions is symmetric. To be more precise, note that the expression \sigma_{u,w}=\nabla_u\circ \nabla_w-\nabla_u w can be considered as a second order differential operator on smooth functions, f\mapsto\sigma_{u,w}f. The value (\sigma_{u,w}f)(a) at each point a depends only on the vectors u(a) and w(a) (the computation is the same as above). The connection is symmetric, if \sigma_{u,w}=\sigma_{w,u} for any two vector fields[9]. This is the condition generalizing the independence of the mixed derivatives on their order.
Connections on Riemannian manifolds
Main article: Levi-Civita connection.
For a connection \nabla defined on the tangent bundle TM of a Riemannian manifold M (with the natural isomorphism between TM and T^*M) it is natural to require certain compatibility between \nabla and the metric structure. This condition can be formulated in several equivalent forms:
- The parallel transport along any curve is an isometric operator;
- The covariant derivative satisfies the Leibniz rule \nabla_w\left< u,v \right>=\left< \nabla_w u,v \right> +\left< u,\nabla_w v \right>, where \nabla_w acts on the function \left< u,w \right> as the usual Lie (directional) derivative;
- The covariant derivative \nabla g of the metric tensor g (in the sense of the derivation of tensors is identically zero.
A "miracle" [Be], also known as the Principal Lemma of Riemannian Geometry [Mi, Lemma 8.6] is the fact that for any Riemannian manifold there is a unique symmetric (torsion-less) connection compatible with the Riemannian metric.
Computational formulas
The proof is given by a straightforward computation in any local coordinates: denoting by g_{ij}=\left<\partial_i,\partial_j \right> the components of the metric tensor[10] and by \Gamma_{ij}^k the Christoffel symbols, we obtain the identities \nabla_{\partial_i}\left<\partial_j,\partial_k\right>=\left<\nabla_{\partial_i}\partial_j,\partial_k\right>+\left<\partial_j,\nabla_{\partial_i}\partial_k\right>, and two other similar identities obtained by cyclical permutation of the indices i,j,k=1,\dots,m, m=\dim M. Thus we have three linear equations with respect to only three unknowns \left<\nabla_{\partial_i}\partial_j,\partial_k\right>,\quad \bigl<\nabla_{\partial_j}\partial_k,\partial_i\bigr>, \quad \left<\nabla_{\partial_k}\partial_i,\partial_j\right> (the remaining terms coincide with one of these because of the symmetry of the scalar product \left< \cdot,\cdot \right> and absence of the torsion, \nabla_{\partial_i}\partial_j=\nabla_{\partial_j}\partial_i).
This system of three equations is immediately solvable, yielding the identity \sum_{\ell}\Gamma_{ij}^\ell g_{\ell k}=\frac12\biggl(\frac{\partial}{\partial b_i}g_{jk}+\frac{\partial}{\partial b_j}g_{ki}+\frac{\partial}{\partial b_k}g_{ij}\biggr). Introducing the symmetric matrix function g^{k\ell} inverse to the metric tensor, we can resolve the above system of linear equations with respect to the Christoffel symbols: \Gamma_{ij}^\ell=\frac12\sum_{k=1}^m \biggl(\frac{\partial}{\partial b_i}g_{jk}+\frac{\partial}{\partial b_j}g_{ki}+\frac{\partial}{\partial b_k}g_{ij}\biggr)g^{k\ell}.\tag{LC} This proves the uniqueness of the connection: its Christoffel symbols are uniquely defined by the components of the metric tensor and their derivatives. One can verify that the connection defined by the above formulas, is indeed compatible with the metric.
Definition. The unique symmetric linear connection compatible with the Riemannian structure on a manifold, is called the Levi-Civita connection.
Example: smooth surfaces in \R^3 and Theorema Egregium
If M is a 2-dimensional smooth surface in \R^3, then it naturally inherits the Riemannian metric from this embedding (vectors tangent to M are also tangent to \R^3 with its flat standard Euclidean structure).
The ambient space also has the natural flat connection: in the canonical coordinates it has zero Cristoffel symbols and the covariant derivative \nabla^\circ=\rd is the coordinate-wise differential: \nabla^\circ_w u=\frac{\rd u}{\rd w}=(L_w u_1,L_w u_2,L_w u_3).
A vector field u tangent to M can be covariantly differentiated along any vector w_a\in T_a M in the sense of the ambient flat connection, but the result in general will be not tangent to M anymore: \nabla^\circ_{w_a}u\in T_a\R^3\smallsetminus T_a M. However, if we apply to \nabla^\circ_w u the orthogonal projection \operatorname{Proj}:T_a\R^3\to T_a M parallel to the unit normal vector field \nu=\{\nu_a\}\perp T_a M, the result will be a well-defined connection on M: the differential operators \nabla=\operatorname{Proj}\circ \nabla^\circ,\qquad \nabla_w u=\frac{\rd u}{\rd w}-\bigl<\frac{\rd u}{\rd w},\nu\bigr>\cdot\nu, will satisfy the Leibniz rule. One can verify by the direct computation, that this connection is compatible with the metric induced on M by its embedding in \R^3.
The Principal Lemma of Riemannian Geometry implies that the curvature of this connection (defined the explicit embedding of M into \R^3) depends in fact only on the "intrinsic" (metric) geometry and is not changed by isometric bending of the surface M. This fact was discovered by Gauss and called by him Theorema Egregium, "the remarkable theorem".
Curvature of a metric
The curvature of the Levi-Civita connection is referred simply as the curvature of the metric. As was mentioned, the curvature defines (and can in turn be characterized) by a family of isometric operators (parallel transport) between two tangent spaces T_a M and T_b M at two different points of M, which depends on a (piecewise) smooth path connecting these points.
In the simplest nontrivial case of 2-surfaces, an isometry corresponding to the parallel transport along a small closed loop \gamma beginning and ending at the specified point a\in M, is a rotation by a small angle depending on the loop (including the orientation of the latter). From the tensorial properties of the curvature it follows that the rotational angle is proportional to the area[11] encircled by the loop. The proportionality coefficient is referred to as the Gauss curvature of a 2-dimensional metric surface at the specified point a.
Note that the Gauss curvature has a sign (positive or negative). In fact, the sign of the curvature (if it is constant for all points of M) is probably the most important local characteristic which affects global properties of the surface, see [Gr].
For Riemannian manifolds of higher dimensions the curvature tensor has several independent components which can be combined in different ways for different purposes, see Ricci curvature.
Other types of connections
As follows from this summary, many physical and geometric constructions can be formalized as connections (or parallel transport) in appropriate bundles (vector or principal). We mention here only the most important particular cases, referring to the Encyclopaedia pages when possible.
- Weyl connection. A connection \nabla on a Riemannian manifold with the metric tensor g, which preserves the conformal structure, i.e., \nabla_w g=\theta g for some positive smooth funcion \theta:M\to\R_+ on M.
- Yang-Mills connection. A connection on a vector bundle over a (pseudo-)Riemannian manifold, whose curvature form is harmonic in the sense of the Hodge-Laplace operator. Plays a key role in the modern physical field theory.
- Symplectic connection. A connection on the tangent space of an even-dimensional symplectic manifold, which preserves the symplectic structure. Unlike the metric connection, is unrelated to any local geometry of the symplectic manifolds (which is trivial by the Darboux theorem) and is never unique.
- Gauss-Manin connection. If \pi:E\to B is a topological bundle with, say, a compact generic fiber F, the fibers F_b=\pi^{-1}(b)\subset E are homeomorphic to each other, although in a non-canonical way. However, for any two sufficiently close points b_1,b_2\in B the fibers F_i=F_{b_i} are homeomorhic and the conjugating homeomorphism is in some sense close to identity. This allows to identify the homology groups H_k(F_1,G) and H_k(F_2,G) in a canonical way for any coefficients group G and all dimensions k=0,1,\dots,\dim F. This identification defines a locally flat connection on the bundle with the same base B and the fibers H_k(\pi^{-1}(b),G). The dual connection is defined on the bundle with the dual fibers H^k(\pi^{-1}(b),G) and is also locally flat. For instance, if G=\R and the cohomology is inderstood in the de Rham sense, a k-form \omega\in\varLambda^k(E) is locally parallel along a path \gamma in the base B, if the restriction of this form on each fiber \pi^{-1}(b) is closed and all periods of this restriction are constant along \gamma. The explicit form of the covariant derivative associated with a Gauss-Manin connection is usually written in the algebraic category.
- Hermitian connection. Defined on bundles whose fibers carry a natural structure of complex Hermitian spaces, in particular, on Hermitian manifolds.
This list should be continued.
Related geometric notions
There are many other geometric notions intimately related to connections. For more details refer to the respective EOM articles.
- Holonomy group. For a given base point a\in B, the holonomy group is the set of all self-maps of the fiber, obtained as parallel transport along closed loops beginning and ending at a. For non-simply connected base B the holonomy group may be nontrivial even for (locally) flat connections.
- Geodesic line (sometimes Geodesic curve or just geodesic). A smooth curve on a Riemannian manifold, whose velocity vector is parallel to itself along the curve. Geodesics are locally shortest paths (provide the minimum of the arc length integral among all curves connecting two sufficiently close points on the geodesic).
- Geodesic curvature, Sectional curvature, Ricci curvature, mean curvature, principal curvature. Various combinations of components of the general metric curvature tensor. One has to distinguish between the intrinsic invariants which depend only on the metric (e.g., induced on an embedded submanifold of a Riemannian manifold) and extrinsic, depending on the embedding itself.
Notes
- ↑ E.g., if the fiber F, is compact, but also if it is a finite-dimensional vector- or G-space with \G' linear or G-invariant.
- ↑ The term linear connection today seems to be used as a complete synonym of the term affine connection.
- ↑ I.e., a tuple of usual, "scalar" 1-forms, of cardinality equal to \dim\mathfrak g.
- ↑ The usual way to write the corresponding formulas explicitly involves canonical \mathfrak g-valued 1-form on the Lie group, associated with the right shift action of G on itself.
- ↑ This term has also other meanings in the theory of linear ordinary differential equations with analytic coefficients, see Stokes phenomenon.
- ↑ Here \rd M(\cdot) is the matrix 1-form on U_{\alpha\beta} whose components are the differentials of the entries of the matrix function M(\cdot).
- ↑ That is, D_\gamma f(b)=\lim_{t\to 0}\frac1t (f(\gamma(t))-f(\gamma(0)): note that scalar functions take values in the same space \R over all points on the curve \gamma.
- ↑ For a general pair of vector fields u,w\in\Gamma (TB), the curvature is defined as [\nabla_u,\nabla_w]-\nabla_{[u,w]}.
- ↑ [Mi, Chapter II, Definition 8.5 and the footnote].
- ↑ By definition, \partial_i=\frac{\partial}{\partial b_i} are the coordinate vector fields on M, and g_{ij}=g_{ji}.
- ↑ The area form is uniquely determined by the Riemannian structure on M^2.
Yakovenko/sandbox1. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Yakovenko/sandbox1&oldid=26929