Lie derivative explained

In differential geometry, the Lie derivative, named after Sophus Lie by Władysław Ślebodziński,[1] [2] evaluates the change of a tensor field (including scalar functions, vector fields and one-forms), along the flow defined by another vector field. This change is coordinate invariant and therefore the Lie derivative is defined on any differentiable manifold.

Functions, tensor fields and forms can be differentiated with respect to a vector field. If T is a tensor field and X is a vector field, then the Lie derivative of T with respect to X is denoted

l{L}XT

. The differential operator

T\mapstol{L}XT

is a derivation of the algebra of tensor fields of the underlying manifold.

The Lie derivative commutes with contraction and the exterior derivative on differential forms.

Although there are many concepts of taking a derivative in differential geometry, they all agree when the expression being differentiated is a function or scalar field. Thus in this case the word "Lie" is dropped, and one simply speaks of the derivative of a function.

The Lie derivative of a vector field Y with respect to another vector field X is known as the "Lie bracket" of X and Y, and is often denoted [''X'',''Y''] instead of

l{L}XY

. The space of vector fields forms a Lie algebra with respect to this Lie bracket. The Lie derivative constitutes an infinite-dimensional Lie algebra representation of this Lie algebra, due to the identity

l{L}[X,Y]T=l{L}Xl{L}YT-l{L}Yl{L}XT,

valid for any vector fields X and Y and any tensor field T.

Considering vector fields as infinitesimal generators of flows (i.e. one-dimensional groups of diffeomorphisms) on M, the Lie derivative is the differential of the representation of the diffeomorphism group on tensor fields, analogous to Lie algebra representations as infinitesimal representations associated to group representation in Lie group theory.

Generalisations exist for spinor fields, fibre bundles with a connection and vector-valued differential forms.

Motivation

A 'naïve' attempt to define the derivative of a tensor field with respect to a vector field would be to take the components of the tensor field and take the directional derivative of each component with respect to the vector field. However, this definition is undesirable because it is not invariant under changes of coordinate system, e.g. the naive derivative expressed in polar or spherical coordinates differs from the naive derivative of the components in Cartesian coordinates. On an abstract manifold such a definition is meaningless and ill defined. In differential geometry, there are three main coordinate independent notions of differentiation of tensor fields: Lie derivatives, derivatives with respect to connections, and the exterior derivative of totally antisymmetric covariant tensors, i.e. differential forms. The main difference between the Lie derivative and a derivative with respect to a connection is that the latter derivative of a tensor field with respect to a tangent vector is well-defined even if it is not specified how to extend that tangent vector to a vector field. However a connection requires the choice of an additional geometric structure (e.g. a Riemannian metric or just an abstract connection) on the manifold. In contrast, when taking a Lie derivative, no additional structure on the manifold is needed, but it is impossible to talk about the Lie derivative of a tensor field with respect to a single tangent vector, since the value of the Lie derivative of a tensor field with respect to a vector field X at a point p depends on the value of X in a neighborhood of p, not just at p itself. Finally, the exterior derivative of differential forms does not require any additional choices, but is only a well defined derivative of differential forms (including functions).

Definition

The Lie derivative may be defined in several equivalent ways. To keep things simple, we begin by defining the Lie derivative acting on scalar functions and vector fields, before moving on to the definition for general tensors.

The (Lie) derivative of a function

Defining the derivative of a function

f\colonM\to{R}

on a manifold is problematic because the difference quotient

style(f(x+h)-f(x))/h

cannot be determined while the displacement

x+h

is undefined.

The Lie derivative of a function

f\colonM\to{R}

with respect to a vector field

X

at a point

p\inM

is the function

(l{L}Xf)(p)={d\overdt}r|t=0l(f\circ

t
\Phi
Xr)(p)

=\limt\to

t
fl(\Phi-fl(pr)
X(p)r)
t
where
t
\Phi
X(p)
is the point to which the flow defined by the vector field

X

maps the point

p

at time instant

t.

In the vicinity of

t=0,

t
\Phi
X(p)
is the unique solution of the system
d
dt

r|t

t
\Phi
X(p)

=

t
Xl(\Phi
X(p)r)
of first-order autonomous (i.e. time-independent) differential equations, with
0
\Phi
X(p)

=p.

Setting

l{L}Xf=\nablaXf

identifies the Lie derivative of a function with the directional derivative, which is also denoted by

X(f):=l{L}Xf=\nablaXf

.

The Lie derivative of a vector field

If X and Y are both vector fields, then the Lie derivative of Y with respect to X is also known as the Lie bracket of X and Y, and is sometimes denoted

[X,Y]

. There are several approaches to defining the Lie bracket, all of which are equivalent. We list two definitions here, corresponding to the two definitions of a vector field given above:

The Lie derivative of a tensor field

Definition in terms of flows

The Lie derivative is the speed with which the tensor field changes under the space deformation caused by the flow.

Formally, given a differentiable (time-independent) vector field

X

on a smooth manifold

M,

let
t
\Phi
X

:M\toM

be the corresponding local flow. Since
t
\Phi
X
is a local diffeomorphism for each

t

, it gives rise to a pullback of tensor fields. For covariant tensors, this is just the multi-linear extension of the pullback map
*
\left(\Phi
p

:

*
T
t
\Phi
X(p)

M\to

*
T
p

M,   

*
\left(\Phi
p

\alpha(X)=\alphal(Tp

t
\Phi
X(X)r),

\alpha\in

*
T
t
\Phi
X(p)

M,X\inTpM

For contravariant tensors, one extends the inverse
-1
\left(T
X\right)

:

T
t
\Phi
X(p)

M\toTpM

t
T
X
. For every

t,

there is, consequently, a tensor field
*
(\Phi
X)

T

of the same type as

T

's.

If

T

is an

(r,0)

- or

(0,s)

-type tensor field, then the Lie derivative

{\calL}XT

of

T

along a vector field

X

is defined at point

p\inM

to be

{\calL}XT(p)=

d
dt

l|t=0

*
\left(l(\Phi
Xr)

T\right)p=

d
dt

l|t=0

*
l(\Phi
p
T
t
\Phi
X(p)

=\limt

*T
l(\Phi-Tp
t
\Phi
X(p)
t

.

The resulting tensor field

{\calL}XT

is of the same type as

T

's.

More generally, for every smooth 1-parameter family

\Phit

of diffeomorphisms that integrate a vector field

X

in the sense that

{d\overdt}r|t=0\Phit=X\circ\Phi0

, one has\mathcal_X T = \bigl(\Phi_0^\bigr)^* \biggr|_ \Phi_t^* T = - \biggr|_ \bigl(\Phi_t^\bigr)^* \Phi_0^* T \, .

Algebraic definition

We now give an algebraic definition. The algebraic definition for the Lie derivative of a tensor field follows from the following four axioms:

Axiom 1. The Lie derivative of a function is equal to the directional derivative of the function. This fact is often expressed by the formula

l{L}Yf=Y(f)

Axiom 2. The Lie derivative obeys the following version of Leibniz's rule: For any tensor fields S and T, we have

l{L}Y(ST)=(l{L}YS)T+S(l{L}YT).

Axiom 3. The Lie derivative obeys the Leibniz rule with respect to contraction:

l{L}X(T(Y1,\ldots,Yn))=(l{L}XT)(Y1,\ldots,Yn)+T((l{L}XY1),\ldots,Yn)++T(Y1,\ldots,(l{L}XYn))

Axiom 4. The Lie derivative commutes with exterior derivative on functions:

[l{L}X,d]=0

If these axioms hold, then applying the Lie derivative

l{L}X

to the relation

df(Y)=Y(f)

shows that

l{L}XY(f)=X(Y(f))-Y(X(f)),

which is one of the standard definitions for the Lie bracket.

The Lie derivative acting on a differential form is the anticommutator of the interior product with the exterior derivative. So if α is a differential form,

l{L}Y\alpha=iYd\alpha+diY\alpha.

This follows easily by checking that the expression commutes with exterior derivative, is a derivation (being an anticommutator of graded derivations) and does the right thing on functions.

Explicitly, let T be a tensor field of type . Consider T to be a differentiable multilinear map of smooth sections α1, α2, ..., αp of the cotangent bundle TM and of sections X1, X2, ..., Xq of the tangent bundle TM, written T(α1, α2, ..., X1, X2, ...) into R. Define the Lie derivative of T along Y by the formula

(l{L}YT)(\alpha1,\alpha2,\ldots,X1,X2,\ldots)=Y(T(\alpha1,\alpha2,\ldots,X1,X2,\ldots))

-T(l{L}Y\alpha1,\alpha2,\ldots,X1,X2,\ldots) -T(\alpha1,l{L}Y\alpha2,\ldots,X1,X2,\ldots)-\ldots

-T(\alpha1,\alpha2,\ldots,l{L}YX1,X2,\ldots) -T(\alpha1,\alpha2,\ldots,X1,l{L}YX2,\ldots)-\ldots

The analytic and algebraic definitions can be proven to be equivalent using the properties of the pushforward and the Leibniz rule for differentiation. The Lie derivative commutes with the contraction.

The Lie derivative of a differential form

See also: Interior product. A particularly important class of tensor fields is the class of differential forms. The restriction of the Lie derivative to the space of differential forms is closely related to the exterior derivative. Both the Lie derivative and the exterior derivative attempt to capture the idea of a derivative in different ways. These differences can be bridged by introducing the idea of an interior product, after which the relationships falls out as an identity known as Cartan's formula. Cartan's formula can also be used as a definition of the Lie derivative on the space of differential forms.

Let M be a manifold and X a vector field on M. Let

\omega\inΛk+1(M)

be a -form, i.e. for each

p\inM

,

\omega(p)

is an alternating multilinear map from

(TpM)k

to the real numbers. The interior product of X and ω is the k-form

iX\omega

defined as

(iX\omega)(X1,\ldots,Xk)=\omega(X,X1,\ldots,Xk)

The differential form

iX\omega

is also called the contraction of ω with X, and
k+1
i
X:Λ

(M)Λk(M)

is a

\wedge

-antiderivation where

\wedge

is the wedge product on differential forms. That is,

iX

is R-linear, and

iX(\omega\wedgeη)=(iX\omega)\wedgeη+(-1)k\omega\wedge(iXη)

for

\omega\inΛk(M)

and η another differential form. Also, for a function

f\inΛ0(M)

, that is, a real- or complex-valued function on M, one has

ifX\omega=fiX\omega

where

fX

denotes the product of f and X.The relationship between exterior derivatives and Lie derivatives can then be summarized as follows. First, since the Lie derivative of a function f with respect to a vector field X is the same as the directional derivative X(f), it is also the same as the contraction of the exterior derivative of f with X:

l{L}Xf=iXdf

For a general differential form, the Lie derivative is likewise a contraction, taking into account the variation in X:

l{L}X\omega=iXd\omega+d(iX\omega).

This identity is known variously as Cartan formula, Cartan homotopy formula or Cartan's magic formula. See interior product for details. The Cartan formula can be used as a definition of the Lie derivative of a differential form. Cartan's formula shows in particular that

dl{L}X\omega=l{L}X(d\omega).

The Lie derivative also satisfies the relation

l{L}fX\omega=fl{L}X\omega+df\wedgeiX\omega.

Coordinate expressions

In local coordinate notation, for a type tensor field

T

, the Lie derivative along

X

is

\begin{align} (l{L}XT)

a1\ldotsar
{}
b1\ldotsbs

={} &

c(\partial
X
c
a1\ldotsar
T
{}
b1\ldotsbs

)\\ &{}-{}(\partialcX

a1

)T

ca2\ldotsar
{}
b1\ldotsbs

-\ldots-(\partialc

ar
X

)T

a1\ldotsar-1c
{}
b1\ldotsbs

\\ &+

(\partial
b1

Xc)T

a1\ldotsar
{}
cb2\ldotsbs

+\ldots+

(\partial
bs

Xc)T

a1\ldotsar
{}
b1\ldotsbs-1c

\end{align}

here, the notation

\partiala=

\partial
\partialxa
means taking the partial derivative with respect to the coordinate

xa

. Alternatively, if we are using a torsion-free connection (e.g., the Levi Civita connection), then the partial derivative

\partiala

can be replaced with the covariant derivative which means replacing

\partialaXb

with (by abuse of notation)

\nablaaXb=

b
X
;a

:=(\nabla

b
X)
a

=\partialaXb+

b
\Gamma
ac

Xc

where the
a
\Gamma
bc

=

a
\Gamma
cb
are the Christoffel coefficients.

The Lie derivative of a tensor is another tensor of the same type, i.e., even though the individual terms in the expression depend on the choice of coordinate system, the expression as a whole results in a tensor

(l{L}XT)

a1\ldotsar
{}
b1\ldotsbs
\partial
a1
⊗ … ⊗ \partial
ar

b1
dx

⊗ … ⊗

bs
dx
which is independent of any coordinate system and of the same type as

T

.

The definition can be extended further to tensor densities. If T is a tensor density of some real number valued weight w (e.g. the volume density of weight 1), then its Lie derivative is a tensor density of the same type and weight.

\begin{align} (l{L}X

a1\ldotsar
T)
{}
b1\ldotsbs

={}

c(\partial
&X
c
a1\ldotsar
T
{}
b1\ldotsbs

)-(\partialcX

a1

)T

ca2\ldotsar
{}
b1\ldotsbs

-\ldots-(\partialc

ar
X

)T

a1\ldotsar-1c
{}
b1\ldotsbs

+\\ &+

(\partial
b1

Xc)T

a1\ldotsar
{}
cb2\ldotsbs

+\ldots+

(\partial
bs

Xc)T

a1\ldotsar
{}
b1\ldotsbs-1c

+w(\partialcXc)T

a1\ldotsar
{}
b1\ldotsbs

\end{align}

Notice the new term at the end of the expression.

\Gamma=(

a
\Gamma
bc

)

, the Lie derivative along

X

is[3]

(l{L}X

a
\Gamma)
bc

=

d\partial
X
d
a
\Gamma
bc

+\partialb\partialcXa-

d
\Gamma
bc

\partialdXa+

a
\Gamma
dc

\partialbXd+

a
\Gamma
bd

\partialcXd

Examples

For clarity we now show the following examples in local coordinate notation.

\phi(xc)\inl{F}(M)

we have:

(l{L}X\phi)=X(\phi)=Xa\partiala\phi

.

Hence for the scalar field

\phi(x,y)=x2-\sin(y)

and the vector field

X=\sin(x)\partialy-

2\partial
y
x
the corresponding Lie derivative becomes \begin\mathcal_X\phi &= (\sin(x)\partial_y - y^2\partial_x)(x^2 - \sin(y))\\ & = \sin(x)\partial_y(x^2 - \sin(y)) - y^2\partial_x(x^2 - \sin(y))\\ & = -\sin(x)\cos(y) - 2xy^2 \\\end

For an example of higher rank differential form, consider the 2-form

\omega=(x2+y2)dx\wedgedz

and the vector field

X

from the previous example. Then,\begin\mathcal_X\omega & = d(i_((x^2 + y^2)dx\wedge dz)) + i_(d((x^2 + y^2)dx\wedge dz)) \\& = d(-y^2(x^2 + y^2) dz) + i_(2ydy\wedge dx\wedge dz) \\& = \left(- 2xy^2 dx + (-2yx^2 - 4y^3) dy\right) \wedge dz + (2y\sin(x)dx \wedge dz + 2y^3dy \wedge dz)\\ & = \left(-2xy^2 + 2y\sin(x)\right)dx\wedge dz + (-2yx^2 - 2y^3)dy\wedge dz\end

Some more abstract examples.

l{L}X(dxb)=diX(dxb)=dXb=\partialaXbdxa

.

Hence for a covector field, i.e., a differential form,

A=

b)dx
A
a(x

a

we have:

l{L}XA=X(Aa)dxa+Abl{L}X(dxb)=(Xb\partialbAa+Ab\partiala(Xb))dxa

The coefficient of the last expression is the local coordinate expression of the Lie derivative.

For a covariant rank 2 tensor field

T=Tab(xc)dxadxb

we have:\begin (\mathcal _X T) &= (\mathcal _X T)_ dx^a\otimes dx^b\\ &= X(T_)dx^a\otimes dx^b + T_ \mathcal_X (dx^c) \otimes dx^b + T_ dx^a \otimes \mathcal_X (dx^c)\\ &= (X^c \partial_c T_+T_\partial_a X^c+T_\partial_b X^c)dx^a\otimes dx^b\\\end

If

T=g

is the symmetric metric tensor, it is parallel with respect to the Levi-Civita connection (aka covariant derivative), and it becomes fruitful to use the connection. This has the effect of replacing all derivatives with covariant derivatives, giving

(l{L}Xg)=(Xcgab;+gcb

c
X
;a

+gac

c
X
;b

)dxadxb=(Xb;a+Xa;b)dxadxb

Properties

The Lie derivative has a number of properties. Let

l{F}(M)

be the algebra of functions defined on the manifold M. Then

l{L}X:l{F}(M)l{F}(M)

is a derivation on the algebra

l{F}(M)

. That is,

l{L}X

is R-linear and

l{L}X(fg)=(l{L}Xf)g+fl{L}Xg.

Similarly, it is a derivation on

l{F}(M) x l{X}(M)

where

l{X}(M)

is the set of vector fields on M (cf. Theorem 6 from the article: Nichita, F.F. Unification Theories: New Results and Examples. Axioms 2019, 8, 60):

l{L}X(fY)=(l{L}Xf)Y+fl{L}XY

which may also be written in the equivalent notation

l{L}X(fY)=(l{L}Xf)Y+fl{L}XY

where the tensor product symbol

is used to emphasize the fact that the product of a function times a vector field is being taken over the entire manifold.

Additional properties are consistent with that of the Lie bracket. Thus, for example, considered as a derivation on a vector field,

l{L}X[Y,Z]=[l{L}XY,Z]+[Y,l{L}XZ]

one finds the above to be just the Jacobi identity. Thus, one has the important result that the space of vector fields over M, equipped with the Lie bracket, forms a Lie algebra.

The Lie derivative also has important properties when acting on differential forms. Let α and β be two differential forms on M, and let X and Y be two vector fields. Then

l{L}X(\alpha\wedge\beta)=(l{L}X\alpha)\wedge\beta+\alpha\wedge(l{L}X\beta)

[l{L}X,l{L}Y]\alpha:=l{L}Xl{L}Y\alpha-l{L}Yl{L}X\alpha=l{L}[X,Y]\alpha

[l{L}X,iY]\alpha=[iX,l{L}Y]\alpha=i[X,Y]\alpha,

where i denotes interior product defined above and it is clear whether [·,·] denotes the commutator or the Lie bracket of vector fields.

Generalizations

Various generalizations of the Lie derivative play an important role in differential geometry.

The Lie derivative of a spinor field

A definition for Lie derivatives of spinors along generic spacetime vector fields, not necessarily Killing ones, on a general (pseudo) Riemannian manifold was already proposed in 1971 by Yvette Kosmann.[4] Later, it was provided a geometric framework which justifies her ad hoc prescription within the general framework of Lie derivatives on fiber bundles[5] in the explicit context of gauge natural bundles which turn out to be the most appropriate arena for (gauge-covariant) field theories.[6]

In a given spin manifold, that is in a Riemannian manifold

(M,g)

admitting a spin structure, the Lie derivative of a spinor field

\psi

can be defined by first defining it with respect to infinitesimal isometries (Killing vector fields) via the André Lichnerowicz's local expression given in 1963:[7]

l{L}X\psi:=Xa\nablaa\psi-

14\nabla
a

Xb\gammaa\gammab\psi,

where

\nablaaXb=\nabla[aXb]

, as

X=Xa\partiala

is assumed to be a Killing vector field, and

\gammaa

are Dirac matrices.

It is then possible to extend Lichnerowicz's definition to all vector fields (generic infinitesimal transformations) by retaining Lichnerowicz's local expression for a generic vector field

X

, but explicitly taking the antisymmetric part of

\nablaaXb

only. More explicitly, Kosmann's local expression given in 1972 is:[4]

l{L}X\psi:=Xa\nablaa\psi-

18\nabla
[a

Xb][\gammaa,\gammab]\psi=\nablaX\psi-

14
(d

X\flat)\psi,

where

[\gammaa,\gammab]=\gammaa\gammab-\gammab\gammaa

is the commutator,

d

is exterior derivative,

X\flat=g(X,-)

is the dual 1 form corresponding to

X

under the metric (i.e. with lowered indices) and

is Clifford multiplication.

It is worth noting that the spinor Lie derivative is independent of the metric, and hence also of the connection. This is not obvious from the right-hand side of Kosmann's local expression, as the right-hand side seems to depend on the metric through the spin connection (covariant derivative), the dualisation of vector fields (lowering of the indices) and the Clifford multiplication on the spinor bundle. Such is not the case: the quantities on the right-hand side of Kosmann's local expression combine so as to make all metric and connection dependent terms cancel.

To gain a better understanding of the long-debated concept of Lie derivative of spinor fields one may refer to the original article,[8] [9] where the definition of a Lie derivative of spinor fields is placed in the more general framework of the theory of Lie derivatives of sections of fiber bundles and the direct approach by Y. Kosmann to the spinor case is generalized to gauge natural bundles in the form of a new geometric concept called the Kosmann lift.

Covariant Lie derivative

If we have a principal bundle over the manifold M with G as the structure group, and we pick X to be a covariant vector field as section of the tangent space of the principal bundle (i.e. it has horizontal and vertical components), then the covariant Lie derivative is just the Lie derivative with respect to X over the principal bundle.

Now, if we're given a vector field Y over M (but not the principal bundle) but we also have a connection over the principal bundle, we can define a vector field X over the principal bundle such that its horizontal component matches Y and its vertical component agrees with the connection. This is the covariant Lie derivative.

See connection form for more details.

Nijenhuis–Lie derivative

Another generalization, due to Albert Nijenhuis, allows one to define the Lie derivative of a differential form along any section of the bundle Ωk(M, TM) of differential forms with values in the tangent bundle. If K ∈ Ωk(M, TM) and α is a differential p-form, then it is possible to define the interior product iKα of K and α. The Nijenhuis–Lie derivative is then the anticommutator of the interior product and the exterior derivative:

l{L}K\alpha=[d,iK]\alpha=

k-1
di
K\alpha-(-1)

iKd\alpha.

History

In 1931, Władysław Ślebodziński introduced a new differential operator, later called by David van Dantzig that of Lie derivation, which can be applied to scalars, vectors, tensors and affine connections and which proved to be a powerful instrument in the study of groups of automorphisms.

The Lie derivatives of general geometric objects (i.e., sections of natural fiber bundles) were studied by A. Nijenhuis, Y. Tashiro and K. Yano.

For a quite long time, physicists had been using Lie derivatives, without reference to the work of mathematicians. In 1940, Léon Rosenfeld[10] —and before him (in 1921[11]) Wolfgang Pauli[12] —introduced what he called a ‘local variation’

\delta\astA

of a geometric object

A

induced by an infinitesimal transformation of coordinates generated by a vector field

X

. One can easily prove that his

\delta\astA

is

-l{L}X(A)

.

See also

References

Notes and References

  1. Book: Trautman, A. . Andrzej Trautman . 2008 . Remarks on the history of the notion of Lie differentiation . Variations, Geometry and Physics: In honour of Demeter Krupka's sixty-fifth birthday . O. . Krupková . D. J. . Saunders . New York . Nova Science . 978-1-60456-920-9 . 297–302 .
  2. Ślebodziński . W. . 1931 . Sur les équations de Hamilton . Bull. Acad. Roy. D. Belg. . 17 . 5 . 864–870 .
  3. Book: Yano, K. . Kentaro Yano (mathematician) . The Theory of Lie Derivatives and its Applications. North-Holland. 1957. 8. 978-0-7204-2104-0.
  4. Kosmann . Y. . Yvette Kosmann-Schwarzbach . 1971 . Dérivées de Lie des spineurs . . 91 . 4 . 317–395 . 10.1007/BF02428822 . 121026516 .
  5. Book: Trautman, A. . 1972 . Invariance of Lagrangian Systems . L. . O'Raifeartaigh . Lochlainn O'Raifeartaigh . General Relativity: Papers in honour of J. L. Synge . Clarenden Press . Oxford . 0-19-851126-4 . 85 .
  6. Book: Fatibene . L. . Francaviglia . M. . Mauro Francaviglia . 2003 . Natural and Gauge Natural Formalism for Classical Field Theories . Kluwer Academic . Dordrecht .
  7. Lichnerowicz . A. . 1963 . Spineurs harmoniques . C. R. Acad. Sci. Paris . 257 . 7–9 .
  8. Book: Fatibene . L. . Ferraris . M. . Francaviglia . M. . Godina . M. . 1996 . A geometric definition of Lie derivative for Spinor Fields . Proceedings of the 6th International Conference on Differential Geometry and Applications, August 28th–September 1st 1995 (Brno, Czech Republic) . Janyska . J. . Kolář . I. . Slovák . J. . Masaryk University . Brno . 549–558 . 80-210-1369-9 . gr-qc/9608003v1 . 1996gr.qc.....8003F .
  9. Godina . M. . Matteucci . P. . 2003 . Reductive G-structures and Lie derivatives . . 47 . 1 . 66–86 . 10.1016/S0393-0440(02)00174-2 . math/0201235 . 2003JGP....47...66G . 16408289 .
  10. Rosenfeld . L. . 1940 . Sur le tenseur d'impulsion-énergie . Mémoires Acad. Roy. D. Belg. . 18 . 6 . 1–30 .
  11. Pauli's book on relativity.
  12. Book: Pauli, W. . Theory of Relativity . First . 1981 . Dover . New York . 1921 . 978-0-486-64152-2 . See section 23