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Levi-Civita connection

From Wikipedia, the free encyclopedia

Affine connection on the tangent bundle of a manifold
A connection on the sphere rolls the tangent plane from one point to another. As it does so, the point of contact traces out a curve in the plane: thedevelopment.

InRiemannian orpseudo-Riemannian geometry (in particular theLorentzian geometry ofgeneral relativity), theLevi-Civita connection is the uniqueaffine connection on thetangent bundle of amanifold thatpreserves the (pseudo-)Riemannian metric and istorsion-free. Thefundamental theorem of Riemannian geometry states that there is a unique connection that satisfies these properties.

The connection formalizes and generalizes the "rolling without slipping or twisting" method of transporting tangent planes of a smooth surface embedded inR3{\displaystyle \mathbb {R} ^{3}} (or generally, any Riemannian manifold, by theNash embedding theorems).

Thecovariant derivative is defined given any affine connection. In the theory ofRiemannian andpseudo-Riemannian manifolds, the "covariant derivative" by default refers to the one defined using the Levi-Civita connection. The components (structure coefficients) of this connection with respect to a system of local coordinates are calledChristoffel symbols.

History

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The Levi-Civita connection is named afterTullio Levi-Civita, although originally "discovered" byElwin Bruno Christoffel. Levi-Civita,[1] along withGregorio Ricci-Curbastro, used Christoffel's symbols[2] to define the notion ofparallel transport and explore the relationship of parallel transport with thecurvature, thus developing the modern notion ofholonomy.[3]

In 1869, Christoffel discovered that the components of the intrinsic derivative of a vector field, upon changing the coordinate system, transform as the components of a contravariant vector. This discovery was the real beginning of tensor analysis.

In 1906,L. E. J. Brouwer was the firstmathematician to consider theparallel transport of avector for the case of a space ofconstant curvature.[4][5]

In 1917,Tullio Levi-Civita pointed out its importance for the case of ahypersurface immersed in aEuclidean space, i.e., for the case of aRiemannian manifold embedded in a "larger" ambient space.[1] He interpreted the intrinsic derivative in the case of an embedded surface as the tangential component of the usual derivative in the ambient affine space. The Levi-Civita notions ofintrinsic derivative and parallel displacement of a vector along a curve make sense on an abstract Riemannian manifold, even though the original motivation relied on a specific embeddingMnRn(n+1)/2.{\displaystyle M^{n}\subset \mathbf {R} ^{n(n+1)/2}.}

In 1918, independently of Levi-Civita,Jan Arnoldus Schouten obtained analogous results.[6] In the same year,Hermann Weyl generalized Levi-Civita's results.[7][8]

Notation

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The metricg can take up to two vectors or vector fieldsX,Y as arguments. In the former case the output is a number, the (pseudo-)inner product ofX andY. In the latter case, the inner product ofXp,Yp is taken at all pointsp on the manifold so thatg(X,Y) defines a smooth function onM. Vector fields act (by definition) as differential operators on smooth functions. In local coordinates(x1,,xn){\displaystyle (x_{1},\ldots ,x_{n})}, the action reads

X(f)=Xixif=Xiif{\displaystyle X(f)=X^{i}{\frac {\partial }{\partial x^{i}}}f=X^{i}\partial _{i}f}

whereEinstein'ssummation convention is used.

Formal definition

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Anaffine connection{\displaystyle \nabla } is called a Levi-Civita connection if

  1. it preserves the metric, i.e.,g=0{\displaystyle \nabla g=0}.
  2. it istorsion-free, i.e., for any vector fieldsX{\displaystyle X} andY{\displaystyle Y} we haveXYYX=[X,Y]{\displaystyle \nabla _{X}Y-\nabla _{Y}X=[X,Y]}, where[X,Y]{\displaystyle [X,Y]} is theLie bracket of thevector fieldsX{\displaystyle X} andY{\displaystyle Y}.

Condition 1 above is sometimes referred to ascompatibility with the metric, and condition 2 is sometimes called symmetry, cf. Do Carmo's text.[9]

Fundamental theorem of (pseudo-)Riemannian geometry

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Main article:Fundamental theorem of Riemannian geometry

Theorem Every pseudo-Riemannian manifold(M,g){\displaystyle (M,g)} has a unique Levi Civita connection{\displaystyle \nabla }.

Proof:[10][11]To prove uniqueness, unravel the definition of the action of a connection on tensors to find

X(g(Y,Z))=(Xg)(Y,Z)+g(XY,Z)+g(Y,XZ){\displaystyle X{\bigl (}g(Y,Z){\bigr )}=(\nabla _{X}g)(Y,Z)+g(\nabla _{X}Y,Z)+g(Y,\nabla _{X}Z)}.

Hence one can write the condition that{\displaystyle \nabla } preserves the metric as

X(g(Y,Z))=g(XY,Z)+g(Y,XZ){\displaystyle X{\bigl (}g(Y,Z){\bigr )}=g(\nabla _{X}Y,Z)+g(Y,\nabla _{X}Z)}.

By the symmetry ofg{\displaystyle g},

X(g(Y,Z))+Y(g(Z,X))Z(g(Y,X))=g(XY+YX,Z)+g(XZZX,Y)+g(YZZY,X){\displaystyle X{\bigl (}g(Y,Z){\bigr )}+Y{\bigl (}g(Z,X){\bigr )}-Z{\bigl (}g(Y,X){\bigr )}=g(\nabla _{X}Y+\nabla _{Y}X,Z)+g(\nabla _{X}Z-\nabla _{Z}X,Y)+g(\nabla _{Y}Z-\nabla _{Z}Y,X)}.

By torsion-freeness, the right hand side is therefore equal to

2g(XY,Z)g([X,Y],Z)+g([X,Z],Y)+g([Y,Z],X){\displaystyle 2g(\nabla _{X}Y,Z)-g([X,Y],Z)+g([X,Z],Y)+g([Y,Z],X)}.

Thus, theKoszul formula

g(XY,Z)=12{X(g(Y,Z))+Y(g(Z,X))Z(g(X,Y))+g([X,Y],Z)g([Y,Z],X)g([X,Z],Y)}{\displaystyle g(\nabla _{X}Y,Z)={\tfrac {1}{2}}{\Big \{}X{\bigl (}g(Y,Z){\bigr )}+Y{\bigl (}g(Z,X){\bigr )}-Z{\bigl (}g(X,Y){\bigr )}+g([X,Y],Z)-g([Y,Z],X)-g([X,Z],Y){\Big \}}}

holds. Hence, if a Levi-Civita connection exists, it must be unique, becauseZ{\displaystyle Z} is arbitrary,g{\displaystyle g} is non degenerate, and the right hand side does not depend on{\displaystyle \nabla }.

To prove existence, note that for given vector fieldX{\displaystyle X} andY{\displaystyle Y}, the right hand side of the Koszul expression is linear over smooth functions in the vector fieldZ{\displaystyle Z}, not just real-linear. Hence by the non degeneracy ofg{\displaystyle g}, the right hand side uniquely defines some new vector field, which is suggestively denotedXY{\displaystyle \nabla _{X}Y} as in the left hand side. By substituting the Koszul formula, one now checks that for all vector fieldsX,Y,Z{\displaystyle X,Y,Z} and all functionsf{\displaystyle f},

g(X(Y1+Y2),Z)=g(XY1,Z)+g(XY2,Z){\displaystyle g(\nabla _{X}(Y_{1}+Y_{2}),Z)=g(\nabla _{X}Y_{1},Z)+g(\nabla _{X}Y_{2},Z)}
g(X(fY),Z)=X(f)g(Y,Z)+fg(XY,Z){\displaystyle g(\nabla _{X}(fY),Z)=X(f)g(Y,Z)+fg(\nabla _{X}Y,Z)}
g(XY,Z)+g(XZ,Y)=X(g(Y,Z)){\displaystyle g(\nabla _{X}Y,Z)+g(\nabla _{X}Z,Y)=X{\bigl (}g(Y,Z){\bigr )}}
g(XY,Z)g(YX,Z)=g([X,Y],Z).{\displaystyle g(\nabla _{X}Y,Z)-g(\nabla _{Y}X,Z)=g([X,Y],Z).}

Hence the Koszul expression does, in fact, define a connection, and this connection is compatible with the metric and is torsion free, i.e. is a Levi-Civita connection.

With minor variation, the same proof shows that there is a unique connection that is compatible with the metric and has prescribed torsion.

Christoffel symbols

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Let{\displaystyle \nabla } be an affine connection on the tangent bundle. Choose local coordinatesx1,,xn{\displaystyle x^{1},\ldots ,x^{n}} with coordinate basis vector fields1,,n{\displaystyle \partial _{1},\ldots ,\partial _{n}} and writej{\displaystyle \nabla _{j}} forj{\displaystyle \nabla _{\partial _{j}}}. TheChristoffel symbolsΓjkl{\displaystyle \Gamma _{jk}^{l}} of{\displaystyle \nabla } with respect to these coordinates are defined as

jk=Γjkll{\displaystyle \nabla _{j}\partial _{k}=\Gamma _{jk}^{l}\partial _{l}}

The Christoffel symbols conversely define the connection{\displaystyle \nabla } on the coordinate neighbourhood because

XY=Xjj(Ykk)=Xjj(Ykk)=Xj(j(Yk)k+Ykjk)=Xj(j(Yk)k+YkΓjkll)=Xj(j(Yl)+YkΓjkl)l{\displaystyle {\begin{aligned}\nabla _{X}Y&=\nabla _{X^{j}\partial _{j}}(Y^{k}\partial _{k})\\&=X^{j}\nabla _{j}(Y^{k}\partial _{k})\\&=X^{j}{\bigl (}\partial _{j}(Y^{k})\partial _{k}+Y^{k}\nabla _{j}\partial _{k}{\bigr )}\\&=X^{j}{\bigl (}\partial _{j}(Y^{k})\partial _{k}+Y^{k}\Gamma _{jk}^{l}\partial _{l}{\bigr )}\\&=X^{j}{\bigl (}\partial _{j}(Y^{l})+Y^{k}\Gamma _{jk}^{l}{\bigr )}\partial _{l}\end{aligned}}}

that is,

(jY)l=jYl+ΓjklYk{\displaystyle (\nabla _{j}Y)^{l}=\partial _{j}Y^{l}+\Gamma _{jk}^{l}Y^{k}}

An affine connection{\displaystyle \nabla } is compatible with a metric iff

i(g(j,k))=g(ij,k)+g(j,ik)=g(Γijll,k)+g(j,Γikll){\displaystyle \partial _{i}{\bigl (}g(\partial _{j},\partial _{k}){\bigr )}=g(\nabla _{i}\partial _{j},\partial _{k})+g(\partial _{j},\nabla _{i}\partial _{k})=g(\Gamma _{ij}^{l}\partial _{l},\partial _{k})+g(\partial _{j},\Gamma _{ik}^{l}\partial _{l})}

i.e., if and only if

igjk=Γijlglk+Γiklgjl.{\displaystyle \partial _{i}g_{jk}=\Gamma _{ij}^{l}g_{lk}+\Gamma _{ik}^{l}g_{jl}.}

An affine connection is torsion free iff

jkkj=(ΓjklΓkjl)l=[j,k]=0.{\displaystyle \nabla _{j}\partial _{k}-\nabla _{k}\partial _{j}=(\Gamma _{jk}^{l}-\Gamma _{kj}^{l})\partial _{l}=[\partial _{j},\partial _{k}]=0.}

i.e., if and only if

Γjkl=Γkjl{\displaystyle \Gamma _{jk}^{l}=\Gamma _{kj}^{l}}

is symmetric in its lower two indices.

As one checks by taking forX,Y,Z{\displaystyle X,Y,Z}, coordinate vector fieldsj,k,l{\displaystyle \partial _{j},\partial _{k},\partial _{l}} (or computes directly), the Koszul expression of the Levi-Civita connection derived above is equivalent to a definition of the Christoffel symbols in terms of the metric as

Γjkl=12glr(kgrj+jgrkrgjk){\displaystyle \Gamma _{jk}^{l}={\tfrac {1}{2}}g^{lr}\left(\partial _{k}g_{rj}+\partial _{j}g_{rk}-\partial _{r}g_{jk}\right)}

where as usualgij{\displaystyle g^{ij}} are the coefficients of the dual metric tensor, i.e. the entries of the inverse of the matrixgkl{\displaystyle g_{kl}}.

Derivative along curve

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The Levi-Civita connection (like any affine connection) also defines a derivative alongcurves, sometimes denoted byD.

Given a smooth curveγ on(M,g) and avector fieldV alongγ its derivative is defined by

DtV=γ˙(t)V.{\displaystyle D_{t}V=\nabla _{{\dot {\gamma }}(t)}V.}

Formally,D is thepullback connectionγ*∇ on thepullback bundleγ*TM.

In particular,γ˙(t){\displaystyle {\dot {\gamma }}(t)} is a vector field along the curveγ itself. Ifγ˙(t)γ˙(t){\displaystyle \nabla _{{\dot {\gamma }}(t)}{\dot {\gamma }}(t)} vanishes, the curve is called a geodesic of the covariant derivative. Formally, the condition can be restated as the vanishing of the pullback connection applied toγ˙{\displaystyle {\dot {\gamma }}}:

(γ)γ˙0.{\displaystyle \left(\gamma ^{*}\nabla \right){\dot {\gamma }}\equiv 0.}

If the covariant derivative is the Levi-Civita connection of a certain metric, then the geodesics for the connection are precisely thosegeodesics of themetric that are parametrised proportionally to their arc length.

Parallel transport

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In general,parallel transport along a curve with respect to a connection definesisomorphisms between the tangent spaces at the points of the curve. If the connection is a Levi-Civita connection, then these isomorphisms areorthogonal – that is, they preserve the inner products on the various tangent spaces.

The images below show parallel transport induced by the Levi-Civita connection associated to two different Riemannian metrics on thepunctured planeR2{0,0}{\displaystyle \mathbf {R} ^{2}\backslash \{0,0\}}. The curve the parallel transport is done along is the unit circle. Inpolar coordinates, the metric on the left is the standardEuclidean metricds2=dx2+dy2=dr2+r2dθ2{\displaystyle ds^{2}=dx^{2}+dy^{2}=dr^{2}+r^{2}d\theta ^{2}}, while the metric on the right isds2=dr2+dθ2{\displaystyle ds^{2}=dr^{2}+d\theta ^{2}}. The first metric extends to the entire plane, but the second metric has a singularity at the origin:

dr=xdx+ydyx2+y2{\displaystyle dr={\frac {xdx+ydy}{\sqrt {x^{2}+y^{2}}}}}
dθ=xdyydxx2+y2{\displaystyle d\theta ={\frac {xdy-ydx}{x^{2}+y^{2}}}}
dr2+dθ2=(xdx+ydy)2x2+y2+(xdyydx)2(x2+y2)2{\displaystyle dr^{2}+d\theta ^{2}={\frac {(xdx+ydy)^{2}}{x^{2}+y^{2}}}+{\frac {(xdy-ydx)^{2}}{(x^{2}+y^{2})^{2}}}}.
Parallel transports on the punctured plane under Levi-Civita connections
Cartesian transport
This transport is given by the metricds2=dr2+r2dθ2{\displaystyle ds^{2}=dr^{2}+r^{2}d\theta ^{2}}.
Polar transport
This transport is given by the metricds2=dr2+dθ2{\displaystyle ds^{2}=dr^{2}+d\theta ^{2}}.

Warning: This is parallel transport on the punctured planealong the unit circle, not parallel transporton the unit circle. Indeed, in the first image, the vectors fall outside of the tangent space to the unit circle.

Example: the unit sphere in R3

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Let⟨ , ⟩ be the usualscalar product onR3. LetS2 be theunit sphere inR3. The tangent space toS2 at a pointm is naturally identified with the vector subspace ofR3 consisting of all vectors orthogonal tom. It follows that a vector fieldY onS2 can be seen as a mapY :S2R3, which satisfiesY(m),m=0,mS2.{\bigl \langle }Y(m),m{\bigr \rangle }=0,\qquad \forall m\in \mathbf {S} ^{2}.

Denote asdmY the differential of the mapY at the pointm. Then we have:

LemmaThe formula(XY)(m)=dmY(X(m))+X(m),Y(m)m{\displaystyle \left(\nabla _{X}Y\right)(m)=d_{m}Y(X(m))+\langle X(m),Y(m)\rangle m}defines an affine connection onS2 with vanishing torsion.

Proof

It is straightforward to prove that satisfies the Leibniz identity and isC(S2) linear in the first variable. It is also a straightforward computation to show that this connection is torsion free. So all that needs to be proved here is that the formula above produces a vector field tangent toS2. That is, we need to prove that for allm inS2(XY)(m),m=0(1).{\displaystyle {\bigl \langle }\left(\nabla _{X}Y\right)(m),m{\bigr \rangle }=0\qquad (1).}Consider the mapf that sends everym inS2 toY(m),m, which is always 0. The mapf is constant, hence its differential vanishes. In particulardmf(X)=dmY(X),m+Y(m),X(m)=0.{\displaystyle d_{m}f(X)={\bigl \langle }d_{m}Y(X),m{\bigr \rangle }+{\bigl \langle }Y(m),X(m){\bigr \rangle }=0.}The equation (1) above follows.Q.E.D.

In fact, this connection is the Levi-Civita connection for the metric onS2 inherited fromR3. Indeed, one can check that this connection preserves the metric.

Behaviour under conformal rescaling

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If the metricg{\displaystyle g} in aconformal class is replaced by the conformally rescaled metric of the same classg^=e2γg{\displaystyle {\hat {g}}=e^{2\gamma }g}, then the Levi-Civita connection transforms according to the rule[12]^XY=XY+X(γ)Y+Y(γ)Xg(X,Y)gradg(γ).{\displaystyle {\widehat {\nabla }}_{X}Y=\nabla _{X}Y+X(\gamma )Y+Y(\gamma )X-g(X,Y)\mathrm {grad} _{g}(\gamma ).}wheregradg(γ){\displaystyle \mathrm {grad} _{g}(\gamma )} is the gradient vector field ofγ{\displaystyle \gamma } i.e. the vector fieldg{\displaystyle g}-dual todγ{\displaystyle d\gamma }, in local coordinates given bygik(iγ)k{\displaystyle g^{ik}(\partial _{i}\gamma )\partial _{k}}. Indeed, it is trivial to verify that^{\displaystyle {\widehat {\nabla }}} is torsion-free. To verify metricity, assume thatg(Y,Y){\displaystyle g(Y,Y)} is constant. In that case,g^(^XY,Y)=X(γ)g^(Y,Y)=12X(g^(Y,Y)).{\displaystyle {\hat {g}}({\widehat {\nabla }}_{X}Y,Y)=X(\gamma ){\hat {g}}(Y,Y)={\frac {1}{2}}X({\hat {g}}(Y,Y)).}

As an application, consider again the unit sphere, but this time understereographic projection, so that the metric (in complexFubini–Study coordinatesz,z¯{\displaystyle z,{\bar {z}}}) is:g=4dzdz¯(1+zz¯)2.{\displaystyle g={\frac {4\,dz\,d{\bar {z}}}{(1+z{\bar {z}})^{2}}}.}This exhibits the metric of the sphere as conformally flat, with the Euclidean metricdzdz¯{\displaystyle dz\,d{\bar {z}}}, withγ=ln(2)ln(1+zz¯){\displaystyle \gamma =\ln(2)-\ln(1+z{\bar {z}})}. We havedγ=(1+zz¯)1(z¯dz+zdz¯){\displaystyle d\gamma =-(1+z{\bar {z}})^{-1}({\bar {z}}\,dz+z\,d{\bar {z}})}, and so^zz=2z¯z1+zz¯.{\displaystyle {\widehat {\nabla }}_{\partial _{z}}\partial _{z}=-{\frac {2{\bar {z}}\partial _{z}}{1+z{\bar {z}}}}.}With the Euclidean gradientgradEuc(γ)=(1+zz¯)1(z¯z+zz¯){\displaystyle \mathrm {grad} _{Euc}(\gamma )=-(1+z{\bar {z}})^{-1}({\bar {z}}\partial _{z}+z\partial _{\bar {z}})}, we have^zz¯=0.{\displaystyle {\widehat {\nabla }}_{\partial _{z}}\partial _{\bar {z}}=0.}These relations, together with their complex conjugates, define the Christoffel symbols for the two-sphere.

See also

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Notes

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  1. ^abLevi-Civita, Tullio (1917)."Nozione di parallelismo in una varietà qualunque" [The notion of parallelism on any manifold].Rendiconti del Circolo Matematico di Palermo (in Italian).42:173–205.doi:10.1007/BF03014898.JFM 46.1125.02.S2CID 122088291.
  2. ^Christoffel, Elwin B. (1869)."Ueber die Transformation der homogenen Differentialausdrücke zweiten Grades".Journal für die reine und angewandte Mathematik.1869 (70):46–70.doi:10.1515/crll.1869.70.46.S2CID 122999847.
  3. ^SeeSpivak, Michael (1999).A Comprehensive introduction to differential geometry (Volume II). Publish or Perish Press. p. 238.ISBN 0-914098-71-3.
  4. ^Brouwer, L. E. J. (1906). "Het krachtveld der niet-Euclidische, negatief gekromde ruimten".Koninklijke Akademie van Wetenschappen. Verslagen.15:75–94.
  5. ^Brouwer, L. E. J. (1906). "The force field of the non-Euclidean spaces with negative curvature".Koninklijke Akademie van Wetenschappen. Proceedings.9:116–133.Bibcode:1906KNAB....9..116B.
  6. ^Schouten, Jan Arnoldus (1918). "Die direkte Analysis zur neueren Relativiteitstheorie".Verhandelingen der Koninklijke Akademie van Wetenschappen te Amsterdam.12 (6): 95.
  7. ^Weyl, Hermann (1918)."Gravitation und Elektrizität".Sitzungsberichte der Königlich Preußischen Akademie der Wissenschaften. Jan-Juni 1918:465–480.Bibcode:1918SPAW.......465W. Reprinted inDas Relativitätsprinzip: Eine Sammlung von Abhandlungen (1923), pp. 147–159,doi:10.1007/978-3-663-19510-8_11,ISBN 978-3-663-19372-2.
  8. ^Weyl, Hermann (1918)."Reine Infinitesimal geometrie".Mathematische Zeitschrift.2 (3–4):384–411.Bibcode:1918MatZ....2..384W.doi:10.1007/bf01199420.S2CID 186232500.
  9. ^Carmo, Manfredo Perdigão do (1992).Riemannian geometry. Francis J. Flaherty. Boston: Birkhäuser.ISBN 0-8176-3490-8.OCLC 24667701.
  10. ^John M Lee (2018).Introduction to Riemannian manifolds. Springer-Verlag. p. 22.
  11. ^Barrett O'Neill (1983).Semi-Riemannian geometry with Applications to relativity. Academic Press. p. 61.
  12. ^Arthur Besse (1987).Einstein manifolds. Springer. p. 58.

References

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