Torsion tensor

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
# )

∇
X

Y
−

∇
Y

X
−
[
X
,
Y
]

{\displaystyle 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). The difference between a connection with torsion, and a corresponding connection without torsion is a tensor, called the contorsion tensor. 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

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

T
(
X
,
Y
)
:=

∇
X

Y
−

∇
Y

X
−
[
X
,
Y
]

{\displaystyle 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 connection which is a first order differential operator: it gives a 2-form on tangent vectors, while the covariant derivative is only defined for vector fields.

### Components of the torsion tensor

The components of the torsion tensor

T
c

a
b

{\displaystyle T^c{}\_{ab} }

 in terms of a local basis (**e**1, ..., **e***n*) of sections of the tangent bundle can be derived by setting *X* = **e***i*, *Y* = **e***j* and by introducing the commutator coefficients *γkij***e***k* := [**e***i*, **e***j*]. The components of the torsion are then

T
k

i
j

:=

Γ
k

i
j

−

Γ
k

j
i

−

γ
k

i
j

,

i
,
j
,
# k
1
,
2
,
…
,
n
.

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

Here

Γ
k

i
j

{\displaystyle {\Gamma^k}\_{ij}}

 are the Christoffel symbols defining the connection. If the basis is holonomic then the Lie brackets vanish,

γ
k

i
j

=
0

{\displaystyle \gamma^k{}\_{ij}=0}

. So

T
k

i
j

=
2

Γ
k

[
i
j
]

{\displaystyle 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

The **torsion form**, an alternative characterization of torsion, applies to the frame bundle F*M* 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 F*M* with the adjoint representation on **gl**(*n*). The frame bundle also carries a canonical one-form θ, with values in **R***n*, defined at a frame *u* ∈ Fx*M* (regarded as a linear function *u* : **R***n* → Tx*M*) by

θ
(
X
# )

u

−
1

(

π

∗

(
X
)
)

{\displaystyle \theta(X) = u^{-1}(\pi\_{\*}(X))}

where *π*  : F*M* → *M* is the projection mapping for the principal bundle and *π∗*  is its push-forward. The torsion form is then

# Θ
d
θ
ω
∧
θ
.

{\displaystyle \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 **R***n*, meaning that under the right action of *g* ∈ Gl(*n*) it transforms equivariantly:

R
g
∗

# Θ

g

−
1

⋅
Θ

{\displaystyle R\_g^\*\Theta = g^{-1}\cdot\Theta}

where *g* acts on the right-hand side through its adjoint representation on **R***n*.

#### Torsion form in a frame

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 (**e**1, ..., **e***n*). The connection form expresses the exterior covariant derivative of these basic sections:

D

e

i

=

e

j

ω
j

i

.

{\displaystyle D\mathbf{e}\_i = \mathbf{e}\_j {\omega^j}\_i .}

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

Θ
k

=
d

θ
k

ω
k

j

∧

θ
j

=

T
k

i
j

θ
i

∧

θ
j

.

{\displaystyle \Theta^k = d\theta^k + {\omega^k}\_j \wedge \theta^j = {T^k}\_{ij} \theta^i \wedge \theta^j.}

In the rightmost expression,

T
k

i
j

=

θ
k

(

∇

e

i

e

j

−

∇

e

j

e

i

−

[

e

i

,

e

j

]

)

{\displaystyle {T^k}\_{ij} = \theta^k\left(\nabla\_{\mathbf{e}\_i}\mathbf{e}\_j - \nabla\_{\mathbf{e}\_j}\mathbf{e}\_i - \left[\mathbf{e}\_i, \mathbf{e}\_j\right]\right)}

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

It can be easily shown that Θ*i* transforms tensorially in the sense that if a different frame

e

~

i

=

e

j

g
j

i

{\displaystyle \tilde{\mathbf{e}}\_i = \mathbf{e}\_j {g^j}\_i}

for some invertible matrix-valued function (*g**j**i*), then

Θ
~

i

=

(

g

−
1

)

i

j

Θ
j

.

{\displaystyle \tilde{\Theta}^i = {\left(g^{-1}\right)^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 T*M*-valued one-form *θ* on *M* corresponding to the identity endomorphism of the tangent bundle under the duality isomorphism End(T*M*) ≈ T*M* ⊗ T∗*M*. Then the torsion two-form is a section

Θ
∈
Hom

(

⋀

2

T

M
,

T

M

)

{\displaystyle \Theta\in\text{Hom}\left({\bigwedge}^2 {\rm T}M, {\rm T}M\right)}

given by

# Θ
D
θ
,

{\displaystyle \Theta = D\theta ,}

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

### Irreducible decomposition

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

i
k

,

{\displaystyle a\_i = T^k{}\_{ik} ,}

and the trace-free part is

B
i

j
k

=

T
i

j
k

1

n
−
1

δ
i

j

a
k

−

1

n
−
1

δ
i

k

a
j

,

{\displaystyle 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
∈
Hom
⁡

(

⋀

2

T

M
,

T

M

)

.

{\displaystyle T\in \operatorname{Hom}\left({\bigwedge}^2 {\rm T}M, {\rm T}M\right).}

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

T
(
X
)
:
Y
↦
T
(
X
∧
Y
)
.

{\displaystyle T(X) : Y \mapsto T(X \wedge Y).}

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

(
tr

T
)
(
X
)

=

def

tr
⁡
(
T
(
X
)
)
.

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

The trace-free part of *T* is then

T
0

=
T
−

1

n
−
1

ι
(
tr

T
)
,

{\displaystyle T\_0 = T - \frac{1}{n-1}\iota(\operatorname{tr} \,T) ,}

where *ι* denotes the interior product.

## Curvature and the Bianchi identities

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

R
(
X
,
Y
)
# Z

∇
X

∇
Y

Z
−

∇
Y

∇
X

Z
−

∇

[
X
,
Y
]

Z
.

{\displaystyle R(X, Y)Z = \nabla\_X\nabla\_YZ - \nabla\_Y\nabla\_XZ - \nabla\_{[X, Y]}Z.}

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. Let

S

{\displaystyle \mathfrak{S}}

 denote the cyclic sum over *X*, *Y*, and *Z*. For instance,

S

(

R

(

X
,
Y

)

Z

)

:=
R
(
X
,
Y
)
Z
R
(
Y
,
Z
)
X
R
(
Z
,
X
)
Y
.

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

Then the following identities hold

1. **Bianchi's first identity:**

S

(

R

(

X
,
Y

)

Z

)

=

S

(

T

(

T
(
X
,
Y
)
,
Z

)

(

∇
X

T

)

(

Y
,
Z

)

)

{\displaystyle \mathfrak{S}\left(R\left(X, Y\right)Z\right) = \mathfrak{S}\left(T\left(T(X, Y), Z\right) + \left(\nabla\_XT\right)\left(Y, Z\right)\right)}
2. **Bianchi's second identity:**

S

(

(

∇
X

R

)

(

Y
,
Z

)

R

(

T

(

X
,
Y

)

,
Z

)

)

=
0

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

### The curvature form and Bianchi identities

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

# ω
d
ω
ω
∧
ω

{\displaystyle \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

1. D
# Θ
Ω
∧
θ

{\displaystyle D\Theta = \Omega \wedge \theta}
2. D
# Ω

{\displaystyle 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 Fx*M*, one has

R
(
X
,
Y
)
Z

=
u

(

2
Ω

(

π

−
1

(
X
)
,

π

−
1

(
Y
)

)

)

(

u

−
1

(
Z
)

)

,

T
(
X
,
Y
)

=
u

(

2
Θ

(

π

−
1

(
X
)
,

π

−
1

(
Y
)

)

)

,

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

where again *u* : **R***n* → Tx*M* 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).

## Characterizations and interpretations

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

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 they experience no acceleration. Suppose that in addition the observer carries with themselves 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

∇

∂

∂
t

∂

∂
x

# x
0

=

{\displaystyle \left.\nabla\_\frac{\partial}{\partial t}\frac{\partial}{\partial x}\right|\_{x=0} = 0.}

Consequently, the torsion is given by

T

(

∂

∂
x

,

∂

∂
t

)

# x
0

=

∇

∂

∂
x

∂

∂
t

# x
0

.

{\displaystyle \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

γ
(
t
)

{\displaystyle \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

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. 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

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

## Geodesics and the absorption of torsion

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

∇

γ
˙

(
t
)

γ
˙

(
t
# )
0

{\displaystyle \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,

γ
˙

(
0
)

{\displaystyle \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.

More precisely, if *X* and *Y* are a pair of tangent vectors at *p* ∈ *M*, then let

Δ
(
X
,
Y
# )

∇
X

Y
~

−

∇
X
′

Y
~

{\displaystyle \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 symmetric and alternating parts of Δ:

S
(
X
,
Y
# )

1
2

(

Δ
(
X
,
Y
)
Δ
(
Y
,
X
)

)

{\displaystyle S(X,Y)=\tfrac12\left(\Delta(X,Y)+\Delta(Y,X)\right)}

A
(
X
,
Y
# )

1
2

(

Δ
(
X
,
Y
)
−
Δ
(
Y
,
X
)

)

{\displaystyle A(X,Y)=\tfrac12\left(\Delta(X,Y)-\Delta(Y,X)\right)}

Then

* A
(
X
,
Y
# )

1
2

(

T
(
X
,
Y
)
−

T
′

(
X
,
Y
)

)

{\displaystyle 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. The difference between these two connections is in fact a tensor, the contorsion tensor.

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.