In
mathematical physics
Mathematical physics refers to the development of mathematics, mathematical methods for application to problems in physics. The ''Journal of Mathematical Physics'' defines the field as "the application of mathematics to problems in physics and t ...
, the gamma
matrices,
, also called the
Dirac matrices, are a set of conventional matrices with specific
anticommutation relations that ensure they
generate a matrix representation of the
Clifford algebra Cl
1,3(
). It is also possible to define
higher-dimensional gamma matrices. When interpreted as the matrices of the action of a set of
orthogonal
In mathematics, orthogonality is the generalization of the geometric notion of '' perpendicularity''.
By extension, orthogonality is also used to refer to the separation of specific features of a system. The term also has specialized meanings in ...
basis vectors for
contravariant vectors in
Minkowski space
In mathematical physics, Minkowski space (or Minkowski spacetime) () is a combination of three-dimensional Euclidean space and time into a four-dimensional manifold where the spacetime interval between any two events is independent of the ...
, the column vectors on which the matrices act become a space of
spinors, on which the Clifford algebra of
spacetime
In physics, spacetime is a mathematical model that combines the three dimensions of space and one dimension of time into a single four-dimensional manifold. Spacetime diagrams can be used to visualize relativistic effects, such as why diffe ...
acts. This in turn makes it possible to represent infinitesimal
spatial rotations and
Lorentz boosts. Spinors facilitate spacetime computations in general, and in particular are fundamental to the
Dirac equation
In particle physics, the Dirac equation is a relativistic wave equation derived by British physicist Paul Dirac in 1928. In its free form, or including electromagnetic interactions, it describes all spin- massive particles, called "Dirac pa ...
for relativistic
spin- particles.
In
Dirac representation, the four
contravariant gamma matrices are
:
is the time-like,
Hermitian matrix. The other three are space-like,
anti-Hermitian matrices. More compactly,
, and
, where
denotes the
Kronecker product and the
(for ) denote the
Pauli matrices.
The gamma matrices have a group structure, the
gamma group, that is shared by all matrix representations of the group, in any dimension, for any signature of the metric. For example, the
Pauli matrices are a set of "gamma" matrices in dimension 3 with metric of Euclidean signature (3, 0). In 5 spacetime dimensions, the 4 gammas above together with the fifth gamma-matrix to be presented below generate the Clifford algebra.
Mathematical structure
The defining property for the gamma matrices to generate a
Clifford algebra is the anticommutation relation
:
where
is the
anticommutator,
is the
Minkowski metric with signature , and
is the
identity matrix
In linear algebra, the identity matrix of size n is the n\times n square matrix with ones on the main diagonal and zeros elsewhere.
Terminology and notation
The identity matrix is often denoted by I_n, or simply by I if the size is immaterial ...
.
This defining property is more fundamental than the numerical values used in the specific representation of the gamma matrices.
Covariant gamma matrices are defined by
:
and
Einstein notation is assumed.
Note that the other
sign convention for the metric, necessitates either a change in the defining equation:
:
or a multiplication of all gamma matrices by
, which of course changes their hermiticity properties detailed below. Under the alternative sign convention for the metric the covariant gamma matrices are then defined by
:
Physical structure
The Clifford algebra over spacetime can be regarded as the set of real linear operators from to itself, , or more generally, when
complexified to , as the set of linear operators from any 4 dimensional complex vector space to itself. More simply, given a basis for , is just the set of all complex matrices, but endowed with a Clifford algebra structure. Spacetime is assumed to be endowed with the Minkowski metric . A space of bispinors, , is also assumed at every point in spacetime, endowed with the
bispinor representation of the
Lorentz group. The bispinor fields of the Dirac equations, evaluated at any point in spacetime, are elements of , see below. The Clifford algebra is assumed to act on as well (by matrix multiplication with column vectors in for all ). This will be the primary view of elements of in this section.
For each linear transformation of , there is a transformation of given by for in . If belongs to a representation of the Lorentz group, then the induced action will also belong to a representation of the Lorentz group, see
Representation theory of the Lorentz group.
If is the
bispinor representation acting on of an arbitrary
Lorentz transformation
In physics, the Lorentz transformations are a six-parameter family of linear transformations from a coordinate frame in spacetime to another frame that moves at a constant velocity relative to the former. The respective inverse transformation i ...
in the standard (4 vector) representation acting on , then there is a corresponding operator on given by equation:
:
showing that the quantity of can be viewed as a ''basis'' of a
representation space
Representation theory is a branch of mathematics that studies abstract algebraic structures by ''representing'' their elements as linear transformations of vector spaces, and studies modules over these abstract algebraic structures. In essen ...
of the
4 vector representation of the Lorentz group sitting inside the Clifford algebra. The last identity can be recognized as the defining relationship for matrices belonging to an
indefinite orthogonal group, which is
written in indexed notation. This means that quantities of the form
:
should be treated as 4 vectors in manipulations. It also means that indices can be raised and lowered on the using the metric as with any 4 vector. The notation is called the
Feynman slash notation
In the study of Dirac fields in quantum field theory, Richard Feynman invented the convenient Feynman slash notation (less commonly known as the Dirac slash notation). If ''A'' is a covariant vector (i.e., a 1-form),
: \ \stackrel\ \gamma^1 A_1 ...
. The slash operation maps the basis of , or any 4 dimensional vector space, to basis vectors . The transformation rule for slashed quantities is simply
:
One should note that this is different from the transformation rule for the , which are now treated as (fixed) basis vectors. The designation of the 4 tuple as a 4 vector sometimes found in the literature is thus a slight misnomer. The latter transformation corresponds to an active transformation of the components of a slashed quantity in terms of the basis , and the former to a passive transformation of the basis itself.
The elements form a representation of the
Lie algebra
In mathematics, a Lie algebra (pronounced ) is a vector space \mathfrak g together with an operation called the Lie bracket, an alternating bilinear map \mathfrak g \times \mathfrak g \rightarrow \mathfrak g, that satisfies the Jacobi iden ...
of the Lorentz group. This is a spin representation. When these matrices, and linear combinations of them, are exponentiated, they are bispinor representations of the Lorentz group, e.g., the of above are of this form. The 6 dimensional space the span is the representation space of a tensor representation of the Lorentz group. For the higher order elements of the Clifford algebra in general and their transformation rules, see the article
Dirac algebra
In mathematical physics, the Dirac algebra is the Clifford algebra \text_(\mathbb). This was introduced by the mathematical physicist P. A. M. Dirac in 1928 in developing the Dirac equation for spin-½ particles with a matrix representation of ...
. The spin representation of the Lorentz group is encoded in the
spin group (for real, uncharged spinors) and in the complexified spin group for charged (Dirac) spinors.
Expressing the Dirac equation
In
natural units
In physics, natural units are physical units of measurement in which only universal physical constants are used as defining constants, such that each of these constants acts as a coherent unit of a quantity. For example, the elementary charge ...
, the Dirac equation may be written as
:
where
is a Dirac spinor.
Switching to
Feynman notation, the Dirac equation is
:
The fifth "gamma" matrix, 5
It is useful to define a product of the four gamma matrices as
, so that
:
(in the Dirac basis).
Although
uses the letter gamma, it is not one of ''the'' gamma matrices of Cl
1,3(
). The number 5 is a relic of old notation, in which
was called "
".
has also an alternative form:
:
using the convention
, or
:
using the convention
.
Proof:
This can be seen by exploiting the fact that all the four gamma matrices anticommute, so
:
,
where
is the type (4,4)
generalized Kronecker delta
In mathematics, the Kronecker delta (named after Leopold Kronecker) is a function of two variables, usually just non-negative integers. The function is 1 if the variables are equal, and 0 otherwise:
\delta_ = \begin
0 &\text i \neq j, \\
1 &\t ...
in 4 dimensions, in full
antisymmetrization. If
denotes the
Levi-Civita symbol in ''n'' dimensions, we can use the identity
.
Then we get, using the convention
,
:
This matrix is useful in discussions of quantum mechanical
chirality. For example, a Dirac field can be projected onto its left-handed and right-handed components by:
:
.
Some properties are:
* It is Hermitian:
*:
* Its eigenvalues are ±1, because:
*:
* It anticommutes with the four gamma matrices:
*:
In fact,
and
are eigenvectors of
since
:
, and
Five dimensions
The
Clifford algebra in odd dimensions behaves like ''two'' copies of the Clifford algebra of one less dimension, a left copy and a right copy. Thus, one can employ a bit of a trick to repurpose as one of the generators of the Clifford algebra in five dimensions. In this case, the set therefore, by the last two properties (keeping in mind that ) and those of the old gammas, forms the basis of the Clifford algebra in spacetime dimensions for the metric signature . In metric signature , the set is used, where the are the appropriate ones for the signature. This pattern is repeated for spacetime dimension even and the next odd dimension for all . For more detail, see
higher-dimensional gamma matrices.
Identities
The following identities follow from the fundamental anticommutation relation, so they hold in any basis (although the last one depends on the sign choice for
).
Miscellaneous identities
1.
2.
3.
4.
5.
6.
, where
Trace identities
The gamma matrices obey the following
trace identities:
Proving the above involves the use of three main properties of the
trace operator:
* tr(''A + B'') = tr(''A'') + tr(''B'')
* tr(''rA'') = ''r'' tr(''A'')
* tr(''ABC'') = tr(''CAB'') = tr(''BCA'')
Normalization
The gamma matrices can be chosen with extra hermiticity conditions which are restricted by the above anticommutation relations however. We can impose
:
, compatible with
and for the other gamma matrices (for )
:
, compatible with
One checks immediately that these hermiticity relations hold for the Dirac representation.
The above conditions can be combined in the relation
:
The hermiticity conditions are not invariant under the action
of a Lorentz transformation
because
is not necessarily a unitary transformation due to the non-compactness of the Lorentz group.
Charge conjugation
The
charge conjugation operator, in any basis, may be defined as
:
where
denotes the
matrix transpose. The explicit form that
takes is dependent on the specific representation chosen for the gamma matrices (its form expressed as product of the gamma matrices is representation dependent, while it can be seen
in the Dirac basis, this fails to hold in the Majorana basis, for example). This is because although charge conjugation is an
automorphism of the
gamma group, it is ''not'' an
inner automorphism
In abstract algebra an inner automorphism is an automorphism of a group, ring, or algebra given by the conjugation action of a fixed element, called the ''conjugating element''. They can be realized via simple operations from within the group i ...
(of the group). Conjugating matrices can be found, but they are representation-dependent.
Representation-independent identities include:
:
In addition, for all four representations given below (Dirac, Majorana and both chiral variants), one has
:
Feynman slash notation
The
Feynman slash notation
In the study of Dirac fields in quantum field theory, Richard Feynman invented the convenient Feynman slash notation (less commonly known as the Dirac slash notation). If ''A'' is a covariant vector (i.e., a 1-form),
: \ \stackrel\ \gamma^1 A_1 ...
is defined by
:
for any 4-vector
.
Here are some similar identities to the ones above, but involving slash notation:
*
*
*
*