Torsion tensor

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Torsion along a geodesic.

In differential geometry, the notion of torsion is a manner of characterizing a twist or screw of a moving frame around a curve. The torsion of a curve, as it appears in the Frenet–Serret formulas, for instance, quantifies the twist of a curve about its tangent vector as the curve evolves (or rather the rotation of the Frenet–Serret frame about the tangent vector). In the geometry of surfaces, the geodesic torsion describes how a surface twists about a curve on the surface. The companion notion of curvature measures how moving frames "roll" along a curve "without twisting".

More generally, on a differentiable manifold equipped with an affine connection (that is, a connection in the tangent bundle), torsion and curvature form the two fundamental invariants of the connection. In this context, torsion gives an intrinsic characterization of how tangent spaces twist about a curve when they are parallel transported; whereas curvature describes how the tangent spaces roll along the curve. Torsion may be described concretely as a tensor, or as a vector-valued two-form on the manifold. If ∇ is an affine connection on a differential manifold, then the torsion tensor is defined, in terms of vector fields X and Y, by

T(X,Y) = \nabla_XY-\nabla_YX - [X,Y]

where [X,Y] is the Lie bracket of vector fields.

Torsion is particularly useful in the study of the geometry of geodesics. Given a system of parametrized geodesics, one can specify a class of affine connections having those geodesics, but differing by their torsions. There is a unique connection which absorbs the torsion, generalizing the Levi-Civita connection to other, possibly non-metric situations (such as Finsler geometry). Absorption of torsion also plays a fundamental role in the study of G-structures and Cartan's equivalence method. Torsion is also useful in the study of unparametrized families of geodesics, via the associated projective connection. In relativity theory, such ideas have been implemented in the form of Einstein–Cartan theory.

The torsion tensor[edit]

Let M be a manifold with a connection ∇ on the tangent bundle. The torsion tensor (sometimes called the Cartan (torsion) tensor) is a vector-valued 2-form defined on vector fields X and Y by

T(X, Y) := \nabla_X Y - \nabla_Y X - [X,Y]

where [X,Y] is the Lie bracket of two vector fields. By the Leibniz rule, T(fX,Y) = T(X,fY) = fT(X,Y) for any smooth function f. So T is tensorial, despite being defined in terms of the non-tensorial covariant derivative: it gives a 2-form on tangent vectors, while the covariant derivative is only defined for vector fields.

Curvature and the Bianchi identities[edit]

The curvature tensor of ∇ is a mapping TM × TM → End(TM) defined on vector fields X, Y, and Z by

R(X,Y)Z = \nabla_X\nabla_YZ - \nabla_Y\nabla_XZ - \nabla_{[X,Y]}Z.

Note that, for vectors at a point, this definition is independent of how the vectors are extended to vector fields away from the point (thus it defines a tensor, much like the torsion).

The Bianchi identities relate the curvature and torsion as follows.[1] Let \mathfrak{S} denote the cyclic sum over X, Y, and Z. For instance,

\mathfrak{S}\left(R(X,Y)Z\right) := R(X,Y)Z + R(Y,Z)X + R(Z,X)Y.

Then the following identities hold

1. Bianchi's first identity:

\mathfrak{S}\left(R(X,Y)Z\right) = \mathfrak{S}\left(T(T(X,Y),Z)+(\nabla_XT)(Y,Z)\right)

2. Bianchi's second identity:

\mathfrak{S}\left((\nabla_XR)(Y,Z)+R(T(X,Y),Z)\right)=0

Components of the torsion tensor[edit]

The components of the torsion tensor  T^c{}_{ab} in terms of a local basis of sections (e1, ..., en) of the tangent bundle can be derived by setting X=ei, Y=ej and by introducing the commutator coefficients γkijek := [ei,ej]. The components of the torsion are then

 T^k{}_{ij} := \Gamma^k{}_{ij} - \Gamma^k{}_{ji}-\gamma^k{}_{ij},\quad i,j,k=1,2,\ldots,n.

If the basis is holonomic then the Lie brackets vanish, \gamma^k{}_{ij}=0. So T^k{}_{ij}=2\Gamma^k{}_{[ij]}. In particular (see below) while the geodesic equations determine the symmetric part of the connection, the torsion tensor determines the antisymmetric part.

The torsion form[edit]

The torsion form, an alternative characterization of torsion, applies to the frame bundle FM of the manifold M. This principal bundle is equipped with a connection form ω, a gl(n)-valued one-form which maps vertical vectors to the generators of the right action in gl(n) and equivariantly intertwines the right action of GL(n) on the tangent bundle of FM with the adjoint representation on gl(n). The frame bundle also carries a canonical one-form θ, with values in Rn, defined at a frame u ∈ FxM (regarded as a linear function u : Rn → TxM) by

\theta(X) = u^{-1}(d\pi(X))

where π  : FMM is the projection mapping for the principal bundle. The torsion form is then

\Theta = d\theta + \omega\wedge\theta.

Equivalently, Θ = Dθ, where D is the exterior covariant derivative determined by the connection.

The torsion form is a (horizontal) tensorial form with values in Rn, meaning that under the right action of g ∈ Gl(n) it transforms equivariantly:

R_g^*\Theta = g^{-1}\cdot\Theta

where g acts on the right-hand side through its fundamental representation on Rn.

The curvature form and Bianchi identities[edit]

The curvature form is the gl(n)-valued 2-form

\Omega = D\omega = d\omega + \omega\wedge\omega

where, again, D denotes the exterior covariant derivative. In terms of the curvature form and torsion form, the corresponding Bianchi identities are[2]

  1. D\Theta = \Omega\wedge\theta
  2. D\Omega = 0.\,

Moreover, one can recover the curvature and torsion tensors from the curvature and torsion forms as follows. At a point u of FxM, one has[3]

R(X,Y)Z = u\left(2\Omega(\pi^{-1}(X),\pi^{-1}(Y))\right)(u^{-1}(Z)),
T(X,Y) = u\left(2\Theta(\pi^{-1}(X),\pi^{-1}(Y))\right),

where again u : Rn → TxM is the function specifying the frame in the fibre, and the choice of lift of the vectors via π−1 is irrelevant since the curvature and torsion forms are horizontal (they vanish on the ambiguous vertical vectors).

Torsion form in a frame[edit]

See also: connection form

The torsion form may be expressed in terms of a connection form on the base manifold M, written in a particular frame of the tangent bundle (e1,...,en). The connection form expresses the exterior covariant derivative of these basic sections:

D{\mathbf e}_i = \sum_{j=1}^n {\mathbf e}_j\omega_i^j.

The solder form for the tangent bundle (relative to this frame) is the dual basis θi ∈ T*M of the ei, so that θi(ej) = δij (the Kronecker delta.) Then the torsion 2-form has components

\Theta^k = d\theta^k + \sum_{j=1}^n\omega^k_j\wedge\theta^j = \sum_{i,j}T_{ij}^k \theta^i\wedge\theta^j.

In the rightmost expression,

T_{ij}^k = \theta^k(\nabla_{\mathbf e_i}\mathbf e_j - \nabla_{\mathbf e_j}\mathbf e_i - [\mathbf e_i,\mathbf e_j])

are the frame-components of the torsion tensor, as given in the previous definition.

It can be easily shown that Θi transforms tensorially in the sense that if a different frame

\tilde{\mathbf e}_i = \sum_j \mathbf e_j g_i^j

for some invertible matrix-valued function (gij), then

\tilde{\Theta}^i = (g^{-1})^i_j\Theta^j.

In other terms, Θ is a tensor of type (1,2) (carrying one contravariant and two covariant indices).

Alternatively, the solder form can be characterized in a frame-independent fashion as the TM-valued one-form θ on M corresponding to the identity endomorphism of the tangent bundle under the duality isomorphism End(TM) ≈ TM ⊗ T*M. Then the torsion two-form is a section of

\Theta\in\text{Hom}(\wedge^2 TM, TM)

given by

\Theta = D\theta,\,

where D is the exterior covariant derivative. (See connection form for further details.)

Irreducible decomposition[edit]

The torsion tensor can be decomposed into two irreducible parts: a trace-free part and another part which contains the trace terms. Using the index notation, the trace of T is given by

a_i = T^k_{ik},

and the trace-free part is

B^i_{jk} = T^i_{jk} + \frac{1}{n-1}\delta^i_ja_k-\frac{1}{n-1}\delta^i_ka_j

where δij is the Kronecker delta.

Intrinsically, one has

T\in \operatorname{Hom}\left(\wedge^2 TM, TM\right).

The trace of T, tr T, is an element of T*M defined as follows. For each vector fixed X ∈ TM, T defines an element T(X) of Hom(TM, TM) via

T(X) : Y \mapsto T(X\wedge Y).

Then (tr T)(X) is defined as the trace of this endomorphism. That is,

(\operatorname{tr}\, T)(X) \stackrel{\text{def}}{=}\operatorname{tr} (T(X)).

The trace-free part of T is then

T_0 = T - \frac{1}{n-1}\iota(\operatorname{tr} \,T)

where ι denotes the interior product.

Characterizations and interpretations[edit]

Throughout this section, M is assumed to be a differentiable manifold, and ∇ a covariant derivative on the tangent bundle of M unless otherwise noted.

Twisting of reference frames[edit]

In the classical differential geometry of curves, the Frenet-Serret formulas describe how a particular moving frame (the Frenet-Serret frame) twists along a curve. In physical terms, the torsion corresponds to the angular momentum of an idealized top pointing along the tangent of the curve.

The case of a manifold with a (metric) connection admits an analogous interpretation. Suppose that an observer is moving along a geodesic for the connection. Such an observer is ordinarily thought of as inertial since she experiences no acceleration. Suppose that in addition the observer carries with herself a system of rigid straight measuring rods (a coordinate system). Each rod is a straight segment; a geodesic. Assume that each rod is parallel transported along the trajectory. The fact that these rods are physically carried along the trajectory means that they are Lie-dragged, or propagated so that the Lie derivative of each rod along the tangent vanishes. They may, however, experience torque (or torsional forces) analogous to the torque felt by the top in the Frenet-Serret frame. This force is measured by the torsion.

More precisely, suppose that the observer moves along a geodesic path γ(t) and carries a measuring rod along it. The rod sweeps out a surface as the observer travels along the path. There are natural coordinates (t,x) along this surface, where t is the parameter time taken by the observer, and x is the position along the measuring rod. The condition that the tangent of the rod should be parallel translated along the curve is

\left.\nabla_{\partial/\partial t}\frac{\partial}{\partial x}\right|_{x=0} = 0.

Consequently, the torsion is given by

\left.T\left(\frac{\partial}{\partial x},\frac{\partial}{\partial t}\right)\right|_{x=0} = \left.\nabla_{\frac{\partial}{\partial x}}\frac{\partial}{\partial t}\right|_{x=0}.

If this is not zero, then the marked points on the rod (the x = constant curves) will trace out helices instead of geodesics. They will tend to rotate around the observer. Note that for this argument it was not essential that \gamma(t) is a geodesic. Any curve would work.

This interpretation of torsion plays a role in the theory of teleparallelism, also known as Einstein-Cartan theory, an alternative formulation of relativity theory.

The torsion of a filament[edit]

In materials science, and especially elasticity theory, ideas of torsion also play an important role. One problem models the growth of vines, focusing on the question of how vines manage to twist around objects.[4] The vine itself is modeled as a pair of elastic filaments twisted around one another. In its energy-minimizing state, the vine naturally grows in the shape of a helix. But the vine may also be stretched out to maximize its extent (or length). In this case, the torsion of the vine is related to the torsion of the pair of filaments (or equivalently the surface torsion of the ribbon connecting the filaments), and it reflects the difference between the length-maximizing (geodesic) configuration of the vine and its energy-minimizing configuration.

Torsion and vorticity[edit]

In fluid dynamics, torsion is naturally associated to vortex lines.

Geodesics and the absorption of torsion[edit]

Suppose that γ(t) is a curve on M. Then γ is an affinely parametrized geodesic provided that

\nabla_{\dot{\gamma}(t)}\dot{\gamma}(t) = 0

for all time t in the domain of γ. (Here the dot denotes differentiation with respect to t, which associates with γ the tangent vector pointing along it.) Each geodesic is uniquely determined by its initial tangent vector at time t=0, \dot{\gamma}(0).

One application of the torsion of a connection involves the geodesic spray of the connection: roughly the family of all affinely parametrized geodesics. Torsion is the ambiguity of classifying connections in terms of their geodesic sprays:

  • Two connections ∇ and ∇′ which have the same affinely parametrized geodesics (i.e., the same geodesic spray) differ only by torsion.[5]

More precisely, if X and Y are a pair of tangent vectors at pM, then let

\Delta(X,Y)=\nabla_X\tilde{Y}-\nabla'_X\tilde{Y}

be the difference of the two connections, calculated in terms of arbitrary extensions of X and Y away from p. By the Leibniz product rule, one sees that Δ does not actually depend on how X and Y' are extended (so it defines a tensor on M). Let S and A be the symmmetric and alternating parts of Δ:

S(X,Y)=\tfrac12\left(\Delta(X,Y)+\Delta(Y,X)\right)
A(X,Y)=\tfrac12\left(\Delta(X,Y)-\Delta(Y,X)\right)

Then

  • A(X,Y) = \tfrac12\left(T(X,Y) - T'(X,Y)\right) is the difference of the torsion tensors.
  • ∇ and ∇′ define the same families of affinely parametrized geodesics if and only if S(X,Y) = 0.

In other words, the symmetric part of the difference of two connections determines whether they have the same parametrized geodesics, whereas the skew part of the difference is determined by the relative torsions of the two connections. Another consequence is:

  • Given any affine connection ∇, there is a unique torsion-free connection ∇′ with the same family of affinely parametrized geodesics.

This is a generalization of the fundamental theorem of Riemannian geometry to general affine (possibly non-metric) connections. Picking out the unique torsion-free connection subordinate to a family of parametrized geodesics is known as absorption of torsion, and it is one of the stages of Cartan's equivalence method.

See also[edit]

Notes[edit]

  1. ^ See Kobayashi–Nomizu (1996) Volume 1, Proposition III.5.2.
  2. ^ Kobayashi–Nomizu (1996) Volume 1, III.2.
  3. ^ Kobayashi–Nomizu (1996) Volume 1, III.5.
  4. ^ Goriely et al. (2006).
  5. ^ See Spivak (1999) Volume II, Addendum 1 to Chapter 6. See also Bishop and Goldberg (1980), section 5.10.

References[edit]