Christoffel symbols


A vector field in ℝn can be seen as a differentiableMathworldPlanetmathPlanetmath (C∞) map V:ℝn→ℝn.

Or as a sectionMathworldPlanetmath ℝn→VT⁢(ℝn) where T⁢ℝn≡ℝn×ℝn is the ℝn’s trivial tangent bundle obeying p↦(p,V(p)∈Tp(ℝn)) with Tp⁢(ℝn)≡ℝn being the tangent spacePlanetmathPlanetmath at p.

Another viewpoint about tangent vectors is that they are also linear operators called derivationsPlanetmathPlanetmath and they act over scalars f:ℝn→ℝ via p↦V⁢f|p=V⁢(p)⋅∇⁡f|p.

Let X be one of them and d⁢X|p its Jacobian matrix evaluated at the point p∈ℝn. Then, for any other vector field Y:ℝn→ℝn,

d⁢X|p⁢(Y⁢(p))

measures how X varies in the direction Y at p.

We have d⁢X|p⁢(Y⁢(p))=(Y⁢(p)⋅∇⁡X1|p,…,Y⁢(p)⋅∇⁡Xn|p), where X=∑sXs⁢es in componentsPlanetmathPlanetmath. Also, it is obvious that p↦d⁢X|p⁢(Y⁢(p)) defines a new vector field in ℝn which is symbolized as

DY⁢X

We can be consider it as a bilinear map

D:T⁢(ℝn)×T⁢(ℝn)→T⁢(ℝn).
(X,Y)↦DX⁢Y

Further, it is easy to see that for any scalar f:ℝn→ℝ

  1. 1.

    Df⁢Y⁢X=f⁢DY⁢X

  2. 2.

    DY⁢(f⁢X)=(Y⁢f)⁢X+f⁢DY⁢X

  3. 3.

    DX⁢Y-DY⁢X=[X,Y]

  4. 4.

    X⁢(Y⋅Z)=DX⁢Y⋅Z+X⋅DX⁢Z

Here we have abbreviated (as usual) Y⁢f=Y⋅∇⁡F and the operationMathworldPlanetmath [X,Y] is the Lie bracketMathworldPlanetmath.

This D is called the standard connectionMathworldPlanetmath of ℝn.

Now, let M be a n-dimensional differentiable manifold and let T⁢M be its tangent bundle. The set of differentiable sections Γ⁢(M)={X:M→T⁢M} is a differentiable Lie algebra which is endowed with a differentiable inner product g:Γ⁢(M)×Γ⁢(M)→ℝ via

g⁢(X,Y)|p=X⁢(p)⋅Y⁢(p)

in each Tp⁢(M)≡ℝn.

It is possible construct a bilinear operator ∇

∇:Γ⁢(M)×Γ⁢(M)→Γ⁢(M)

compatibleMathworldPlanetmath with g and which satisfies the following properties

  1. 1.

    ∇f⁢Y⁡X=f⁢∇Y⁡X

  2. 2.

    ∇Y⁡(f⁢X)=(Y⁢f)⁢X+f⁢∇Y⁡X

  3. 3.

    ∇X⁡Y-∇Y⁡X=[X,Y]

  4. 4.

    X⁢g⁢(Y,Z)=g⁢(∇X⁡Y,Z)+g⁢(X,∇X⁡Z)

The Fundamental Theorem of Riemannian Geometry establishes that this ∇ exists and it is unique, and it is called the Levi-Civita connectionMathworldPlanetmath for the metric g on M.

Now, if one uses a coordinated patch in M one has a set of n-coordinated vector fields ∂1,..,∂n meaning ∂i=∂∂⁡ui being ui the coordinate functions. These are also dubbed holonomic derivations.

So it makes sense to speak about the derivativesPlanetmathPlanetmath ∇∂i⁡∂j and since the ∂i are tangentPlanetmathPlanetmathPlanetmath which generate at a point Tp⁢(M), then ∇∂i⁡∂j is also tangent, so there are n×n numbers (functions if one varies position) Γi⁢js which enters in the relationMathworldPlanetmath

∇∂i⁡∂j=∑sΓi⁢js⁢∂s.

These coefficientsMathworldPlanetmath Γi⁢js are called Christoffel symbolsMathworldPlanetmath and an easy calculation shows that

Γi⁢jk=12⁢∑sgk⁢s⁢[gs⁢j,i+gi⁢s,j-gi⁢j,s]

where gi⁢j=g⁢(∂i,∂j), gi⁢j are the entries of the matrix [gi⁢j]-1 and gi⁢j,k=∂k⁡(gi⁢j).

Routinely one can check that under a change of coordinates ui→wj these functions transform as

Γ¯k⁢li=∂⁡wi∂⁡um⁢∂⁡un∂⁡wk⁢∂⁡up∂⁡wl⁢Γn⁢pm+∂2⁡up∂⁡wk⁢∂⁡wl⁢∂⁡wi∂⁡up

here we have used Einstein’s sum convention (m,n,p-sums) and the term

∂2⁡up∂⁡wk⁢∂⁡wl⁢∂⁡wi∂⁡up

shows that the Γk⁢li are not tensors.

For a proof please see the last part in: http://planetmath.org/?op=getobj&from=collab&id=64http://planetmath.org/?op=getobj&from=collab&id=64

Connection with base vectors.

Let us assume that coordinates ui are referred to a right-handed orthogonalMathworldPlanetmathPlanetmathPlanetmath Cartesian system with attached constant base vectors 𝐞i≡𝐞i and coordinates wj referred to a general curvilinear system attached to a local covariant base vectors 𝐠j and local contravariant base vectors 𝐠k, both systems embedded in the Euclidean space ℝn. We shall also suppose diffeomorphic the transfomation ui↦wj. Then, by definition

𝐠j:=∂⁡ui∂⁡wj⁢𝐞i,𝐠j:=∂⁡wj∂⁡ui⁢𝐞i, (1)

and its inversesPlanetmathPlanetmathPlanetmathPlanetmathPlanetmath

𝐞i=𝐞i=∂⁡ui∂⁡wj⁢𝐠j=∂⁡wj∂⁡ui⁢𝐠j. (2)

Let us consider differentiationMathworldPlanetmath of base vectors 𝐠j, which may be written from (1),(2)

∂⁡𝐠j∂⁡wk=∂2⁡ui∂⁡wj⁢∂⁡wk⁢𝐞i=∂2⁡ui∂⁡wj⁢∂⁡wk⁢∂⁡ui∂⁡ws⁢𝐠s=∂2⁡ui∂⁡wj⁢∂⁡wk⁢∂⁡ws∂⁡ui⁢𝐠s≡∂⁡𝐠k∂⁡wj,

and using the Christoffel symbols this becomes

∂⁡𝐠j∂⁡wk=Γj⁢k⁢s⁢𝐠s=Γj⁢kr⁢𝐠r, (3)

where

Γj⁢k⁢s=∂2⁡ui∂⁡wj⁢∂⁡wk⁢∂⁡ui∂⁡ws,Γj⁢kr=gr⁢s⁢Γj⁢k⁢s. (4)

Since the transformationMathworldPlanetmath of covariant and contravariant metric tensorsMathworldPlanetmath are given by

gj⁢k=∂⁡ui∂⁡wj⁢∂⁡ul∂⁡wk⁢δi⁢l,gj⁢k=∂⁡wj∂⁡ui⁢∂⁡wk∂⁡ul⁢δi⁢l,

is easy to see from here that Christoffel symbol Γj⁢k⁢s enjoy the property

Γj⁢k⁢s=12(∂⁡gj⁢s∂⁡wk+∂⁡gk⁢s∂⁡wj-∂⁡gj⁢k∂⁡ws)⋅ (5)

In a similarMathworldPlanetmathPlanetmathPlanetmath way we find for the derivative of the contravariant base vectors

∂⁡𝐠j∂⁡wk=-Γk⁢sj⁢𝐠s. (6)

Is easy to show the following results:

Γj⁢k⁢s=Γk⁢j⁢s=𝐠s⋅∂⁡𝐠k∂⁡wj=𝐠s⋅∂⁡𝐠j∂⁡wk,
Γj⁢kr=Γk⁢jr=𝐠r⋅∂⁡𝐠j∂⁡wk=𝐠r⋅∂⁡𝐠k∂⁡wj=-𝐠j⋅∂⁡𝐠r∂⁡wk,
Γi⁢ri=12⁢gi⁢s⁢(gi⁢s,r+gr⁢s,i-gi⁢r,s)=12⁢gi⁢s⁢gi⁢s,r=12⁢g⁢∂⁡g∂⁡gi⁢s⁢∂⁡gi⁢s∂⁡wr=1g⁢∂⁡g∂⁡wr,
Γj⁢s⁢k+Γk⁢s⁢j=gj⁢k,s,

comma denoting differentiation with respect to the curvilinear coordinates wj and g=|gj⁢k|. When the coordinate curves are orthogonal we have the following formulae for the Christoffel symbols: (repeated indices are not to be summed)

Γj⁢k⁢s=0,Γj⁢ks=0,(j≠k≠s≠j),
Γi⁢i⁢r=-12∂⁡gi⁢i∂⁡wr,Γi⁢ir=-12⁢gr⁢r∂⁡gi⁢i∂⁡wr,(r≠i),
Γi⁢r⁢i=Γr⁢i⁢i=12∂⁡gi⁢i∂⁡wr,Γr⁢ir=Γi⁢rr=12⁢gr⁢r∂⁡gr⁢r∂⁡wi=12∂⁡log⁡gr⁢r∂⁡wi⋅
Title Christoffel symbols
Canonical name ChristoffelSymbols
Date of creation 2013-03-22 15:43:52
Last modified on 2013-03-22 15:43:52
Owner juanman (12619)
Last modified by juanman (12619)
Numerical id 24
Author juanman (12619)
Entry type Definition
Classification msc 53B20
Classification msc 53-01
Synonym connection coefficients
Related topic Connection