The Z3-graded extension of the Poincar\'e algebra
Richard Kerner

TL;DR
This paper constructs a Z3-graded extension of the Poincaré algebra, involving an extended 12-dimensional space-time with complex-valued metrics, and explores its representations and symmetry properties.
Contribution
It introduces a novel Z3-graded extension of the Poincaré algebra requiring a 12-dimensional space-time with complex metrics, expanding the algebraic framework of relativistic symmetries.
Findings
Extended 12D Minkowski space-time with complex metrics
Representation via differential operators and Casimir operators
Discussion of symmetry properties of the generalized algebra
Abstract
A Z3 symmetric generalization of the Dirac equation was proposed in recent series of papers, where its properties and solutions discussed. The generalized Dirac operator acts on "coloured spinors" composed out of six Pauli spinors, describing three colours and particle-antiparticle degrees of freedom characterizing a single quark state, thus combining Z2 x Z_2 x Z_3 symmetries of 12-component generalized wave functions. Spinorial representation of the Z3-graded generalized Lorentz algebra was introduced, leading to the appearance of extra Z2 x Z2 x Z3 symmetries, probably englobing the symmetries of isospin, flavors and families. The present article proposes a construction of Z3-graded extension of the Poincar\'e algebra. It turns out that such a generalization requires introduction of extended 12-dimensional Minkowskian space-time containing the usual 4-dimensional space-time as a…
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The -graded extension of the Poincaré algebra
Richard Kerner
Abstract
A symmetric generalization of the Dirac equation was proposed in [2], [3], and its properties and solutions discussed in [4], [5]. The generalized Dirac operator acts on coloured spinors composed out of six Pauli spinors, describing three colours and particle-antiparticle degrees of freedom characterizing a single quark state, thus combining symmetries of -component generalized wave functions. The -graded generalized Lorentz algebra and its spinorial representation were introduced in [10], leading to the appearance of extra symmetries, probably englobing the symmetries of isospin, flavors and families.
The present article proposes the construction of -graded extension of the Poincaré group. It turns out that such a generalization requires introduction of extended -dimensional Minkowskian space-time containing the usual -dimensional space-time as a subspace, and two other mutually conjugate “replicas” with complex-valued vectors and metric tensors. Representation in terms of differential operators and generalized Casimir operators are introduced and their symmetry properties are briefly discussed.
Laboratoire de Physique Théorique de la Matière Condensée (LPTMC), Sorbonne - Universités - CNRS UMR 7600 Tour 23-13, 5-ème étage, Boîte Courrier 121, 4 Place Jussieu, 75005 Paris, FRANCE
1 Introduction
There can be little doubt that of all symmetries displayed by physics of elementary particles and fields, the invariance under the action of discrete groups are by far the best confirmed by the experiment, and also the most fundamental. The simplest discrete group is , the group of permutations of two objects. These permutations are cyclic, therefore the same group can be interpreted as . Such an identification is no more possible for the next permutation group, , which contains six elements, out of which only the cyclic ones form a three-dimensional subgroup .
The cyclic group plays crucial role in quantum physics of particles and fields. Its two representations in complex plane, implemented as symmetries of arguments of complex wave functions, the trivial one and the faithful one, lead to different fundamental statictics creating the great divide between two quantum statistics characterizing bosons and fermions. In the space of functions depending on two arguments, we can have two dfferent behaviors with repsect to the permutations;
[TABLE]
The relationship between the spin and statistics is another illustration of importance of discrete symmetries. It establishes a one-to-one dependence between the ireeducible representations of the Lorentz group and the two possible statistical behaviors defined by (1): half-integer spin representations for fermions, and integer spin representations for bosons.
The Dirac equation for the electron provides and example of entaglement of two apparently independent symmetries. The discovery of dichotomic spin parameter which in the case of the electron can take on only two exclusive values led Pauli to the conclusion that a Schödinger-like equation for the electron should involve a two-component wave function:
[TABLE]
where denotes the three Pauli matrices, which form the basis of traceless hermitian matrices, and is the momentum operator, with . This equation does not satisfy the Lorentz-invariant condition: iterating it leads to wrong relation between energy, momentum and mass, instead of , which made Pauli abandon this version introducing the approximate non-relativistic equation for the electron interacting with electromagnetic field [6].
It turns out that relativistic covariance can be restored via introduction of another two-component Pauli spinor, the two similar equation intertwining them with mass terms of opposite sign. Let the two Pauli spinors be denoted by and . Then the following system of equations satisfies relativistic dispersion relation, and is Lorentz covariant:
[TABLE]
which is Dirac’s equation in a less usual basis.[7]. By iterating it, we get the relativistic condition satisfied bu both Pauli spinors: . In the more familiar form, the same system is written in a manifestly relativistic form, with the -component Dirac spinor composed of two Pauli spinors and , and the Dirac matrices expressed in terms of tensor products of matrices as follows:
[TABLE]
The Dirac equation is invariant with respect to symmetry. The first concerns the spin of the electron, which can have two projections on the momentum; the second group, imposed by the requirement of Lorentz invariance, concerns the particle-antiparticle symmetry.
Recently in [1], [2], [3], [4] a generalization of the Dirac equation for quarks was proposed, incorporating the color degrees of freedom via extending the discrete symmetry of the system to the group. The cyclic group is generated by the third root of unity, denoted by , with , , and . Just as taking into account the dichotomic half-integer spin variable, the introduction of color degrees of freedom requires additional symmetry acting on a new discrete variable taking three possible (and exclusive) values, named symbolically “red”, “blue” and “green”. The matrices had to be introduced, all representing third roots of the unit matrix. Six Pauli spinors represent three colors and three anti-colors:
[TABLE]
on which Pauli sigma-matrices act in a natural way. By analogy with the pair of equations (3) in which multiplying the mass by led to the anti-particle appearance, now the mass term is multipleid by the generator of the group, , each time the colour changes. This yields the following set of what may be called the ”colour Dirac equation”:
[TABLE]
[TABLE]
[TABLE]
In an appropriate basis, the system (6) can be represented in a Dirac-like form as follows:
[TABLE]
where is the generalized -component spinor made of Pauli spinors (5), and the generalized Dirac matrices are constructed as follows:
[TABLE]
where
[TABLE]
The two traceless matrices and are both cubic roots of unit matrix. They generate the entire Lie algebra of the group.
The system (7) becomes diagonal only after sixth iteration, yielding the dispersion relation of sixth order:
[TABLE]
This expression is not manifestly relativistic invariant, but it represents a unique light cone multiplied by a positive form-factor:
[TABLE]
Such field theories of higher order were considered by T.D.Lee and G.Wick [8] and were recently an object of renewed interest [9].
The colour Dirac matrices defined in (8) do not span the usual Clifford algebra, and do not transform as relativistic -vectors under ordinary Lorentz transformations. In order to implement Lorentz covariance, the set of -matrices must be extended up to six different realizations, forming doublets transforming under the extension of the Lorentz algebra, containing the usual Lorentz algebra as subalgebra, and two conjugate replicas forming a -graded algebra acting on the generalized multi-spinors formed by six -dimensional colour Dirac spinors, the total dimension of the representation space being (see the details in [10]. The multiplication rules in are -graded, i.e. one has .
The aim of the present article is to define a similar -graded extension of the Poincaré algebra realized in terms of differential operators acting on an extended Minkowskian space-time.
2 The symmetry
Let us recall briefly the properties of the cyclic () and the permutation () groups of three elements. Their representation in terms of rotations and reflections in the complex plane are shown in the following Figure 1:
Let us denote by and the two complex third roots of unity, given by
[TABLE]
satisfying obvious identities so that ,
The six symmetry transformations contain the identity, two rotations, one by , another one by , and three reflections, in the -axis, in the -axis and in the -axis. The subgroup contains only the three rotations. Odd permutations must be represented by idempotents, i.e. by operations whose square is the identity operation. We can make the following choice:
[TABLE]
Here the bar denotes the complex conjugation, i.e. the reflection in the real line, the hat denotes the reflection in the root , and the star the reflection in the root . The six operations close in a non-abelian group with six elements, which are represented as rotation and reflexion operation in the complex plane, as shown in (1) above.
In what follows, we shall use the group for grading of linear spaces and matrix algebras [11], [12], [1]. The -graded algebras are composed of three vector subspaces, one of which (of -grade zero) constitutes a subalgebra in the ordinary sense:
[TABLE]
The multiplication in the graded algebra (14) obeys the following scheme:
[TABLE]
The symmetry can be combined with the symmetry; and being prime numbers, the Cartesian product of the two is isomorphoic with another cyclic group, . The generalized Dirac equation is invariant under the discrete group (which is not isomorphic with because is not a prime number, being divisible by and by ).
The cyclic group is represented in the complex plane by its generator , and its powers from to . In terms of the group generated by and group generated by , we have
[TABLE]
as shown in the figure (2) below.
In analogy with colours labeling quark fields, if the “white” combination is represented by [math], then we have two linear colourless sums of three powers of , namely and , and three white combinations of colour with its anti-colour, , just like a fermion and its antiparticle, or three bosons (like e.g. mesons and ).
A -graded analog of Pauli’s exclusion principle was introduced and its algebraic and physical consequences investigated in [2], [5].
3 The -extended Minkowskian spacetime
Let us denote by the standard four-dimensional Minkowskian spacetime, a -dimensional real vector space endpwed with pseudo-Euclidean (Minkowskian) metric . A spacetime vector is given by its coordinates in a chosen orthonormal frame:
[TABLE]
often replaced by a more practical notation with small Greek indices running from [math] to :
[TABLE]
The three replicas of a -vector will be labeled with the superscripts relative to the elements of the -group as follows:
[TABLE]
In each of the three sectors the specific quadratic form is given, defining the group of transformations keeping it invariant:
[TABLE]
which leads to the following explicit expressions of as functions of and ():
[TABLE]
Let us denote the three quadratic forms, one real and two mutually complex conjugate, by the following three tensors
[TABLE]
defined on each of the subspaces of the generalized Minkowskian space
[TABLE]
The superscripts refer to the -grades attributed to each of the three subspaces. These grades will play an important role in defining the -graded extension of the Poincaré algebra acting on the extended Minkowskian space-time . We should underline here that the three “replicas” are to be treated as really independent components of the resulting -dimensional manifold. For convenience, we shall use the same letters designing three types of space-time components, labeling them with an extra index as follows:
[TABLE]
Idempotent operators projecting on one of the three subspaces of the generalized Minkowskian space-time can be constructed using the matrices and introduced in (9) as follows. Let us define two matrices acting on :
[TABLE]
Then the following three projection operators can be formed:
[TABLE]
One checks easily that and for .
Interesting higher-dimensional and complex extensions of Minkowskian space-time were investigated in [13], [14], albeit without introducing the grading.
4 The -graded Lorentz group
The quadratic Minkowskian square of the vector , is invariant under the transformations of the Lorentz group. The space rotations touching only the -dimensional vector leave all the three quadratic expressions invariant, because they depend only on its -dimensional Euclidean square ; therefore we can fix our attention at the Lorentzian boosts. As we can always align the relative velocity along one of the orthonormal axes of the chosen inertial frame, say , those boosts can be considered only between the time and the coordinates. Here are the three matrices representing the same Lorentz boost (with real parameter equal to ) leaving invariant one of the three quadratic invariants given in (19):
[TABLE]
The three matrices are self-adjoint:
[TABLE]
The above matrices transform each of the three sectors of the -Minkowski space into itself, which founds its reflection in the lower indices is quite transparent: transforms a vector belonging to the [math]-th sector of the -graded Minkowskian space into a -vector belonging to the same sector, and similarly for the matrix operators and .
It is also easy to prove that each set is a representation of a one-parameter subgroup representing a particular Lorentz boost, here between the time variable (hereafter always represented by ) and one cartesian coordinate, say . For example, the product of two Lorentz boosts acting on the sector , is a boost of the same type:
[TABLE]
and similarly for a product of two boosts acting on the sector ,
[TABLE]
The full set of three independent “classical” (i.e. belonging to the subgroup denoted by ) Lorentz boosts is given by three matrices, with independent parameters :
[TABLE]
To make the extension of the Lorentz boosts complete we need also two sets of complementary matrix operators transforming one sector into another. There are two types of such operators, one raising the index of each subspace, another lowering the index by . It is quite easy to find out their matrix representation.
The matrices lowering the index by are::
[TABLE]
The determinant of each of these matrices is equal to . The matrices raising the index by one (or decreasing it by , which is equivalent from the point of view of the -grading) are:
[TABLE]
The determinant of each of these matrices is equal to . The above sets of three matrices each, decreasing and raising the index, are mutually hermitian adjoint:
[TABLE]
Here again, the logic of the lower indices is quite transparent: a matrix labeled transforms a -vector belonging to the sector into a -vector belonging to the sector , and so forth, e.g.:
[TABLE]
The matrices raising or lowering the -grade of the particular type of the -vector they are acting on do not form a group, because most of the products of two such matrices produce new matrices not belonging to the set defined above. However, inside each of one-parameter families corresponding to a given choice of the single space direction concerned by the Lorentz boost, or displays the group property if the products are taken according to the chain rule, with second index of the first factor equal to the first index of the second factor, like in the following examples:
[TABLE]
The above matrices represent a reduced version of Lorentz boosts with relative velocity aligned on the unique axis . As in the previous case, the full versions are given by the following three matrices corresponding to the three independent Lorentz boosts. The boosts of the increasing type, transforming -vectors from sector to [math], from sector to and from sector [math] to , respectively, are as follows:
- the three boosts are given by:
[TABLE]
- the three boosts are given by:
[TABLE]
and the three boosts are given by:
[TABLE]
The boosts of the decreasing type, transforming -vectors from sector to [math], from sector to and from sector [math] to , respectively, are as follows:
- the three boosts are given by:
[TABLE]
- the three boosts are given by:
[TABLE]
and the three boosts are given by:
[TABLE]
The nine matrices , act on the -extended Minkowskian vector in a specifically ordered way. Let us write a -extended vector as a column with entries, composed of three -vectors belonging each to one of the -graded sectors:
[TABLE]
[TABLE]
It is easy to see that the so defined matrices display not only the group property, but also the grading in the following sense:
[TABLE]
In other words, the elements of three subsets of the -graded group of boosts behave under associative matrix multiplication as folows:
[TABLE]
The three sets of matrices ordered in the particular blocks (42) form a three-parameter family which can be considered as the extension of the set of three independent Lorentz boosts. In order to obtain the extension of the entire Lorentz group including the -parameter subgroup of space rotations we shall first investigate the -graded infinitesimal generators of the Lorentz boosts, and then, taking their commutators, define the -graded extension of the space rotations.
5 The -graded Lorentz algebra
The -graded matrix Lie algebra corresponding to the -graded Lie group defined above is easily obtained by taking the differentials of corresponding families of generators of -parameter abelian subgroups in the vicinity of the unit element (corfresponding to the [math] value of the parameter , , etc.). It is sufficient to develop all terms in a Taylor series of powers of the parameter and keep only linear terms in the formulae for the matrices of the Lie group defined above, which means that the terms like or will be suppressed, and the terms with will be replaced by . Thus, we define:
- the full set of three independent “classical” generators (i.e. belonging to the subgroup acting in the first sector of the -extended Mikowski space and which we shall denote and , the three matrices, defining the boosts between the variables and , respectively: acting in the first sector of the -extended Mikowski space
[TABLE]
as well as two similar sets of matrices, denoted respectively and , acting in the sectors and of the -extended Minkowskian space transforming them onto themselves:
[TABLE]
transforming the sector onto itself, and
[TABLE]
transforming sector onto itself.
There are also the two sets of complementary matrix operators transforming sectors into one another. There are two types of such infinitesimal generators, one raising the index of each subspace, another decreasing the index by . Their matrix representation is as follows:
- the infinitesimal generators of three boosts are given by:
[TABLE]
- the three infinitesimal generators of boosts are given by:
[TABLE]
and the three boosts are given by:
[TABLE]
The boosts of the increasing type, transforming -vectors from sector [math] to , from sector to and from sector to [math], respectively, are as follows:
- the three infinitesimal boosts are given by:
[TABLE]
- the three boosts are given by:
[TABLE]
and the three boosts are given by:
[TABLE]
The so defined infinitesimal generators keep the symmetry properties of the Lie group matrices, i.e. they close under the commutator product, provided that the two factors satisfy the chain rule, with the second index of the first matrix coinciding with the first index of the second matrix, like in the following examples:
[TABLE]
The generators form three groups containing three matrices each, belonging to raising, lowering or neutral type with respect to the -grade of the Minkowskian -vector
[TABLE]
Each of the three big matrices composed of three blocks of matrices () appears in three different versions corresponding to the choice of one of the three elementary Lorentz boosts in or -dimensional spacetime planes. Let us denote them by , corresponding to the respective choice of the space direction or . For example, for we shall get explicitly
[TABLE]
and so forth.
The spatial rotations around the axes and are represented in the usual -dimensional Minkowskian space as follows:
[TABLE]
The full set of matrices representing three independent spatial rotations acting on the twelve-dimensional -graded Minkowskian spacetime is as follows:
[TABLE]
They also form a graded Lie algebra with respect to the ordinary Lie bracket (the commutator of matrices). Therefore we get the full set of -graded relations defining the algebra ( are modulo ), conformally with the structure of the -graded Lorentz algebra introduced in [10].
[TABLE]
6 -extended Poincaré algebra and the Casimir operators
The standard Poincaré algebra is the semi-direct product of the Lorentz algebra and the -dimensional abelian algebra of translations , satisfying the well-known commutation relations:
[TABLE]
[TABLE]
In terms of six generators and , , the standard commutation relations
[TABLE]
must be complemented by the following extra commutation relations with :
[TABLE]
The most appropriate realization of the totality of commutation relations given by (59) and (62) is via differential operators, with the generators identified with partial derivations . These operators can be produced from the standard matrix representation by the following well-known procedure. Let us take for example the matrix representation of -dimensional rotations given by formulae (57). The differential operators corresponding to and are obtained by taking formally the scalar product of the space-time -covector with the -gradient transformed by the corresponding matrix . Take for example the matrix :
[TABLE]
Similarly we get
Our next aim is to extend the standard Poincaré algebra so as to include the -graded Lorentz algebra defined by the set of commutation relations (59) complemented by the set of three types of translation generators, denoted by , and . Let us separate time and space components; we shall write then
[TABLE]
We expect the following -graded generalization of standard commutation relations between the Lorentz and translation generators:
[TABLE]
[TABLE]
[TABLE]
In all the above relations the grades add up modulo .
The construction of differential operators providing faithful representation of the -graded Poincaré algebra (67) we shall follow the prescription given by (63) with matrices introduced in previous section, and -component generalizations of Minkowskian -vectors and co-vectors. Let us introduce the following notation for generalized vectors in triple Minkowskian space-time:
[TABLE]
The notations are obvious: the lower index “[math]” refers to the standard Minkowskian component (graded [math]), while the indices “” and “” refer to two complex extensions, mutually conjugate, of grades and , respectively.
For the moment we leave aside the definition of metrics in the so extended triple Minkowskian space-time.
Partial derivatives take, with respect to these variables are represented by the following -component column vector (written here as a horizontal co-vector transposed, in order to spare the space):
[TABLE]
What is left now is to compute patiently the results of contraction of the co-vector (68) with the -component generator of generalized translations (69) with one of the eighteen matrices representing the generalized Lorentz algebra (59) sandwiched in between. This will produce the generators of the -graded Poincaré algebra represented in form of linear differential operators. With twelve translations (64) we shall get the -dimensional -graded extension of the Poincaré algebra, of which the usual -dimensional subalgebra is the standard Poincaré algebra.
The results are a bit cumbersome, but their construction and symmetry properties are quite clear.
Let us start with the nine generalized Lorentz boosts . We have explicitly:
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
The -graded generalized differential operators representing the Lorentz boosts display remarkable symmetry properties. The “diagonal” generators are hermitian: they are invariant under the simultaneous complex conjugation, replacing by and vice versa, and switching the indices .
Under the same hermitian symmetry operation the -graded boosts and transform into each other, so that we have
[TABLE]
The commutation relations between the generalized Lorentz boosts given by (70, 71) and (72) define the differential representation of -graded extension of pure rotations, , with and . By tedious (but not too sophisticated) calculation we can check that the commutation relations between the -graded Lorentz boosts imposed as hypothesis in (59):
[TABLE]
lead indeed to the following expressions for spatial rotations :
[TABLE]
[TABLE]
[TABLE]
Note that the above generators are sums of classical expressions for , each of them acting in its own sector of the -graded extension of Minkowskian space-time.
The grade generators of rotations have the same form, but mix up coordinates with derivatives from different sectors, in cyclical order, symbolically :
[TABLE]
[TABLE]
[TABLE]
Finally, the grade generators of spatial rotations, , repeat the same scheme, but in reverse (anti-cyclic) order, i.e. :
[TABLE]
[TABLE]
[TABLE]
It can easily be checked that these differential operators correspond to what we would get by direct construction using the matrix representation given in (58). The differential operators acting on the -graded extension of Minkowskian space-time; the generalized Lorentz boosts and the generalized space rotations , with and , define the faithful representation of the -graded generalization of the Lorentz group.
In order to introduce the extension to full Poincaré group we have to add three -component generators of translations each one acting on its own sector of the generalized -graded Minkowskian space-time. It turns out that in order to satisfy the -graded set of standard commutation relations given by (67), the three differential operators
[TABLE]
must be defined as follows:
[TABLE]
[TABLE]
[TABLE]
It can be checked by direct computation that the eighteen generators and together with the twelve generalized -graded translations defined above by (76, 77, 78) satisfy the full set of -graded extension of the Poincaré algebra. Its total dimension is , three times ten, corresponding to three replicas of the classical Poincaré group, one “diagonal”, acting on three components of the -graded Minkowskian space-time without mixing them, and two other replicas acting on all three components transforming them into one another. The commutations relations are given by the set defined in (64, 65, 66) and (67).
Classical Poincaré algebra admits two Casimir operators which commute with all generators. These are the -square of the translation -vector , and the -square of the Pauli-Lubanski -vector , where
[TABLE]
In terms of more familiar generators and the Pauli-Lubanski vector takes on the following form:
[TABLE]
The following relations are easily verified:
[TABLE]
The eigenvalues of these two Casimir operators, corresponding to the mass and orbital spin of a given particle state, define the irreducible representations of the Poincaré group,
[TABLE]
In the case of the -graded extension the corresponding Casimir operators must be invariant under permutations imposed by the symmetry. That is to say, the three types of generators should contribute equally to the generalized Casimir operator. The expression generalizing the mass operator should contain not only the obvious term , but also other contributions of all possible grades, like e.g. another grade [math] term: , as well as other similar terms of grades and . The symmetric and real combination imitating the first Casimir operator in (82) is as follows:
[TABLE]
The Pauli-Lubanski -vector also possesses its -graded extensions. They are of the following form:
[TABLE]
[TABLE]
[TABLE]
With these three graded Pauli-Lubanski vectors we can produce a -invariant extended Casimir operator of orbital spin:
[TABLE]
The analysis of eigenvalues of the generalized Casimir operators and the classification of irreducible representations of -graded extension of the Poincaré algebra presented here will be the subject of the forthcoming publications.
Acknowledgement The author is greatly indebted to Jerzy Lukierski for countless discussions, enlightening remarks and lots of very useful suggestions.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[1] R. Kerner, O. Suzuki, The discrete quantum origin of the Lorentz group and the Z 3-graded ternary algebras , Proceedings of the RIMS Conference on Mathematical Physics, Kyoto 2013, pp. 54-72 (2014) see also: https://ci.nii.ac.jp/naid/110009863886
- 2[2] R. Kerner, Ternary generalization of Pauli’s principle and the Z 6 subscript 𝑍 6 Z_{6} -graded algebras , Physics of Atomic Nuclei , 80 (3), pp. 529-531 (2017). also: ar Xiv:1111.0518, ar Xiv:0901.3961
- 3[3] R. Kerner, in Mathematical Structures and Applications , Springer, pp. 311-357 (2018)
- 4[4] R. Kerner, Ternary Z 2 × Z 3 subscript 𝑍 2 subscript 𝑍 3 Z_{2}\times Z_{3} graded algebras and ternary Dirac equation , Physics of Atomic Nuclei 81 (6), pp. 871-889 (2018), also: ar Xiv:1801.01403
- 5[5] R. Kerner, The Quantum nature of Lorentz invariance , Universe , 5 (1), p.1, (2019). https://doi.org/10.3390/universe 5010001 (2019)
- 6[6] W. Pauli, Zeitschrift für Physik , 26 (5), pp. 336-363 (1926)
- 7[7] P.A.M. Dirac, Proc. Royal Soc. A , 117 (778), pp. 610-624 (1928)
- 8[8] T.D. Lee and G.C. Wick, Phys. Rev. D , 2 p. 1033 (1970)
