Today, we are going to talk about the Lie groups and , and their respective Lie algebras, generally denoted by and by the physics community. In addition to this, we will see some properties of the orthogonal groups in euclidean “signature” and general quadratic metrics due to their importance in special relativity or its higher dimensional analogues.

Let us remember what kind of groups are and :

1) The unitary group is defined by:

2) The special unitary group is defined by:

The group operation is the usual matrix multiplication. The respective algebras are denoted as we said above by and . Moreover, if you pick an element , there exists an hermitian (antihermitian if you use the mathematician “approach” to Lie algebras/groups instead the convention used mostly by physicists) matrix such that:

Some general properties of unitary and special unitary groups are:

1) and are compact Lie groups. As a consequence, they have unitary, finite dimensional and irreducible representations. and are subgroups of if .

2) Generators or parameters of unitary and special unitary groups. As we have already seen, the unitary group has parameters (its “dimension”) and it has rank (its number of Casimir operators). The special unitary group has free parameters (its dimension) and it has rank (its number of Casimir operators).

3) Lie algebra generators. The unitary group has a Lie algebra generated by the space of dimensional complex matrices. The special unitary group has a Lie algebra generated by the dimensional space of hermitian traceless matrices.

4) Lie algebra structures. Given a basis of generators for the Lie algebra, we define the constants , , by the following equations:

These structure constants are totally antisymmetric under the exchange of any two indices while the coefficients are symmetric under those changes. Moreover, we also have:

**Remark(I): **From , we get , and from here we can prove the statement 3) above.

**Remark(II):** An arbitrary element of can be expressed as a product of an element of and an element of . That is, we can write , where the symbol means “group isomorphism”.

**Example 1.** The SU(2) group.

In particular, for , we get

This is an important group in physics! It appears in many contexts: angular momentum (both classical and quantum), the rotation group, spinors, quantum information theory, spin networks and black holes, the Standard Model, and many other places. So it is important to know it at depth. The number of parameters of SU(2) is equal to 3 and its rank is equal to one (1). As generators of the Lie algebra associated to this Lie group, called su(2), we can choose for free 3 any independent traceless (trace equal to zero) matrices. As a convenient choice, it is usual to select the so called Pauli matrices :

In general, these matrices satisfy an important number of mathematical relations. The most important are:

and

The commutators of Pauli matrices are given by:

The structure constants read

The Casimir operator/matrix related to the Pauli basis is:

This matrix, by Schur’s lemma, has to be a multiple of the identity matrix (it commutes with each one of the 3 generators of the Pauli algebra, as it can be easily proved). Please, note that using the previous Pauli representation of the Pauli algebra we get:

Q.E.D.

A similar relation, with different overall prefactor, must be true for ANY other representation of the Lie group algebra su(2). In fact, it can be proved in Quantum Mechanics that this number is “four times” the quantum number associated to the angular momentum and it characterizes completely the representation. The general theory of the representation of the Lie group SU(2) and its algebra su(2) is known in physics as the general theory of the angular momentum!

**Example 2.** The SU(3) group.

If n=3, the theory of is important for Quantum Chromodynamics (QCD) and the quark theory. It is also useful in Grand Unified Theories (GUTs) and flavor physics.

The number of parameters of SU(3) is 8 (recall that there are 8 different massless gluons in QCD) and the rank of the Lie algebra is equal to two, so there are two Casimir operators.

The analogue generators of SU(3), compared with the Pauli matrices, are the so-called Gell-Mann matrices. They are 8 independent traceless matrices. There are some “different” elections in literature, but a standard choice are the following matrices:

Gell-Mann matrices above satisfy a normalization condition:

where is the Kronecker delta in two indices.

The two Casimir operators for Gell-Mann matrices are:

1)

This operator is the natural generalization of the previously seen SU(2) Casimir operator.

2)

Here, the values of the structure constans and for the su(3) Lie algebra can be tabulated in rows as follows:

1) For we have .

2) If

then have

**Example 3.** Euclidean groups, orthogonal groups and the Lorentz group in 4D and general dimensional analogues.

In our third example, let us remind usual galilean relativity. In a 3D world, physics is the same for every inertial observer (observers moving with constant speed). Moreover, the fundamental invariant of “motion” in 3D space is given by the length:

In fact, with tensor notation, the above “euclidean” space can be generalized to any space dimension. For a ND space, the fundamental invariant reads:

Mathematically speaking, the group leaving the above metrics invariant are, respectively, SO(3) and SO(N). They are Lie groups with dimensions and , respectively and their Lie algebra generators are antisymmetric traceless and matrices. Those metrics are special cases of quadratic forms and it can easily proved that orthogonal transformations with metric (the euclidean metric given by a Kronecker delta tensor) are invariant in the following sense:

or equivalently

using matric notation. In special relativity, the (proper) Lorentz group is composed by every real matrix connected to the identity through infinitesimal transformations, and the Lorentz group leaves invariant the Minkovski metric(we use natural units with ):

if you use the “mostly plus” 3+1 metric () or, equivalentaly

if with a “mostly minus” 1+3 metric ().

These equations can be also generalized to arbitrary signature. Suppose there are s-spacelike dimensions and t-time-like dimensions (). The associated non-degenerated quadratic form is:

In matrix notation, the orthogonal rotations leaving the above quadratic metrics are said to belong to the group (or is you use the mostly minus convention) real orthogonal group over the corresponding quadratic form. The signature of the quadratic form is said to be or (equivalently and with the alternative convention). We are not considering “degenerated” quadratic forms for simplicity of this example. The Lorentzian or Minkovskian metric are invariant in the same sense that the euclidean example before:

The group has signature or or in non-degenerated quadratic spaces. Obviously, the rotation group is a subgroup of and more generally is a subgroup of . We are going to focus now a little bit on the common special relativity group . This group have 6 parameters or equivalently its group dimension is 6. The rank of this special relativity group is equal to 1. We can choose as parameters for the group 3 spatial rotation angles and three additional parameters, that we do know as rapidities . These group generators have Lie algebra generators and or more precisely, if we define the Lorentz boosts as

In the case of , a possible basis for the Lie algebra generators are the next set of matrices:

And the commutation rules for these matrices are given by the basic relations:

**Final remark:** are sometimes called isometry groups since they define isometries over quadratic forms, that is, they define transformations leaving invariant the “spacetime length”.

Hello,

I think that in your formula for the second Casimir operator for the Gell-Mann matrice you have forgotten some terms (may be proportional to because of what you say after?

I mean the formula for ,

If could you complete it it would be great! Thanks in advance,

Ezequiel. (sequi76@gmail.com)

I think you are wrong…See page 2 of the following pdf for details or any book about group theoryhttp://theory.gsi.de/~friman/e-part-script/EPP_11.pdf

Of course, there are many other Casimirs, but these two are specially useful…

Regards

Amarashiki

Hi Amarashiki,

thanks for your prompt reply. I have put that formula to obtain the explicit form of the operator in the 3-representation and it does not commute with all the Gell-Mann matrices. Only with the and the . It should commute with all of them, right?

See the notebook,

http://users.df.uba.ar/sequi/bajador/casimir_SU3.nb

I have verified the entries 3 times, may be not enough….? Thanks, all the best,

Ezequiel.

Please, see this too…The Casimir C(3) is OK as it is written here. Please, check the matrix elements and your numerical procedure. A summary here http://scipp.ucsc.edu/~haber/ph251/gellmann13.pdf