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(Clifford d rtdit rsne scheme. presented into orated xmt ymty h addition The symmetry. oximate toue pnms formula spin-mass ntroduced soet aeanwlo at look new a take to one ws ain.I oesense, some In tations. no lmnaypril as particle elementary of on onjugation mt) hsoeainclosely operation This imate). h SU( the re wihalapproximate, all (which tries sion fiaino pc-ieand space-time of ification T P P ,ms spectrum mass s, iereversal time , N r eeae by generated are -hois h first The )-theories. C gba This lgebra. rsnstefirst the presents attrans- xact lud- C a be can T and SU(3) of the three light quarks. The addition of the b quark (bottom) extends the quark model to SU(5) with a very approximate symmetry. It is obvious that the next step in extending the flavor symmetry to SU(6) is senseless, since the existence of baryons witha t quark (top) is very unlikely due to the short lifetime of the top-quark. However, there is an idea (which takes its origin from sixties) to consider exact space-time transformations and approximate internal symmetries within one theoretical framework. As is known, elementary particles can be grouped into multiplets corresponding to irreducible representations of so-called algebras of internal symmetries (for example, multiplets of the isospin algebra su(2) or multiplets of the algebra su(3)). Particles from the fixed multiplet have the same parity and the same spin, but they can be distinguished by the masses. Thus, an algebra of the most general symmetry cannot be defined as a direct sum P ⊕ S of two ideals, where P is the Poincar´ealgebra and S is the algebra of internal symmetry, since in contrary case all the particle masses of the multiplet should be coincide with each other. One possible way to avoid this obstacle is the searching of a more large algebra L that contains P and S as subalgebras in such way that µ if only one generator from S commutes with P . In this case a mass operator pµp is not invariant of the large algebra L. Hence it follows that a Cartan subalgebra H should be commute with P , since eigenvalues of the basis elements Hi of H ∈ S are used for definition of the states in multiplets (hypercharge, I3-projection of the isospin and so on). All these quantum numbers are invariant under action of the Poincar´egroup P. Therefore, if L is the Lie algebra spanned on the basis elements of the Poincar´ealgebra P and on the basis elements of the semisimple algebra S, then L can be defined as a direct sum of two ideals, L = P ⊕ S, only in the case when [P,H] = 0, where H is the Cartan subalgebra of S. When the algebra of internal symmetry is an arbitrary compact algebra K (for example, su(2), su(3), ..., su(n), ...) we have the following direct sum: K = N ⊕ S = N ⊕ S1 ⊕ S2 ⊕ ... ⊕ Sn, where N is a center of the algebra K, S is a semisimple algebra, and Si are simple algebras (see [1]). In this case the large algebra L can be defined also as a direct sum of two ideals, L = P ⊕ K, when [P,C] = 0, where C is a maximal commutative subalgebra in K. Restrictions [P,H] = 0 and [P,C] = 0 on the algebraic level induce restrictions on the group level. So, if G is an arbitrary Lie group, and S (group of internal symmetry) and P = T4 ⊙ SL(2, C) (Poincar´egroup) are the subalgebras of G such that any g ∈ G has an unique decomposition in the product g = sp, s ∈ S, p ∈ P, and if there exists one element g ∈ P, −1 g 6∈ T4, such that s gs ∈ P for all s ∈ S, then G = P ⊗ S [2]. The restrictions L = P ⊕ S (algebraic level) and G = P ⊗S (group level) on unification of space-time and internal symmetries were formulated in sixties in the form of so-called no-go theorems. One of the most known no-go theorem is a Coleman-Mandula theorem [3]. The group G is understood in [3] as a symmetry group of S matrix. The Coleman-Mandula theorem asserts that G is necessarily locally isomorphic to the direct product of an internal symmetry group and the Poincar´egroup, and this theorem is not true if the local isomorphism (G≃P⊗S) is replaced by a global isomorphism. In 1966, Pais [4] wrote: ”Are there any alternatives left to the internal symmetry⊗Poincar´egroup picture in the face of the no-go theorems?”. All the no-go theorems suppose that space-time continuum is a fundamental level of reality. However, in accordance with Penrose twistor programme [5, 6], space-time continuum is a deriva- tive construction with respect to underlying spinor structure. Spinor structure contains in itself pre-images of all basic properties of classical space-time, such as dimension, signature, metrics and many other. In parallel with twistor approach, decoherence theory [7] claims that in the background of reality we have a nonlocal quantum substrate (quantum domain), and all visible world (classical domain) arises from quantum domain in the result of decoherence process [8, 9]. In this context space-time should be replaced by the spinor structure (with the aim to avoid re- strictions of the no-go theorems), and all the problem of unification of space-time and internal symmetries should be transferred to a much more deep level of the quantum domain (underlying
2 spinor structure). This article presents one possible way towards a unification of spinor structure and internal symmetries. At first, according to Wigner [10] an elementary particle is defined by an irreducible unitary representation of the Poincar´egroup P. On the other hand, in accordance with SU(3)- theory (and also flavor-spin SU(6)-theory) an elementary particle is described by a vector of irreducible representation of the group SU(3) (SU(6), ..., SU(N), ...). For example, in a so-called ‘eightfold way’ [11] hadrons (baryons and mesons) are grouped within eight-dimensional regular 0 representation Sym(1,1) of SU(3). With the aim to make a bridge between these interpretations 0 0 (between representations of P and vectors of Sym(1,1), Sym(1,4), ...) we introduce a spin-charge S Q Hilbert space H ⊗ H ⊗ H∞, where the each vector of this space presents an irreducible repre- sentation of the group SL(2, C). At this point, charge characteristics of the particles are described by a pseudoautomorphism of the spinor structure. An action of the pseudoautomorphism allows one to distinguish charged and neutral particles within separated charge multiplets. On the other hand, spin characteristics of the particles are described via a generalized notion of the spin based on the spinor structure and irreducible representations of the group SL(2, C). The usual definition of the spin is arrived at the restriction of SL(2, C) to the subgroup SU(2). This construction allows us to define an action and representations of internal symmetry groups SU(2), SU(3), ... in the S Q space H ⊗ H ⊗ H∞ by means of a central extension. In this context the SU(3)-theory is con- sidered in detail. The fermionic and bosonic octets, which compound the eightfold way of SU(3), and also their SU(3)/ SU(2)-reductions into isotopic multiplets are reformulated without usage of the quark scheme. It is well known that the quark model does not explain a mass spectrum of elementary particles. The Gell-Mann–Okubo mass formula explains only mass splitting within supermultiplets of the SU(3)-theory, namely, hypercharge mass splitting within supermultiplets and charge splitting within isotopic multiplets belonging to a given supermultiplet. The analogous situation takes place in the case of B´eg-Singh mass formula of the flavor-spin SU(6)-theory. On the other hand, in nature we see a wide variety of baryon octets (see, for example, Particle Data Group: pdg.lbl.gov), where mass distances between these octets are not explained by the quark model. Hence it follows that mass spectrum of elementary particles should be described by a such parameter that defines relation between mass and spin. With this aim in view we introduce a relation between mass and spin in the section 2. It is shown that for representations (l, l˙) of the Lorentz group the mass is proportional to (l +1/2)(l˙ +1/2), and particles with the same spin but distinct masses are described by different representations of Lorentz group. The introduced mass formula defines basic mass terms, and detailed mass spectrum is accomplished by charge and hypercharge mass splitting via the Gell-Mann–Okubo mass formula (like Zeeman effect in atomic spectra).
2 Complex momentum
A universal covering of the proper orthochronous Lorentz group SO0(1, 3) (rotation group of the Minkowski space-time R1,3) is the spinor group
α β α β Spin (1, 3) ≃ ∈ C : det =1 = SL(2, C). + γ δ 2 γ δ
Let g → Tg be an arbitrary linear representation of the proper orthochronous Lorentz group A SO0(1, 3) and let i(t) = Tai(t) be an infinitesimal operator corresponding to the rotation ai(t) ∈ B SO0(1, 3). Analogously, let i(t) = Tbi(t), where bi(t) ∈ G+ is the hyperbolic rotation. The
3 elements Ai and Bi form a basis of Lie algebra sl(2, C) and satisfy the relations
[A1, A2]= A3, [A2, A3]= A1, [A3, A1]= A2, [B , B ]= −A , [B , B ]= −A , [B , B ]= −A , 1 2 3 2 3 1 3 1 2 A B A B A B [ 1, 1]=0, [ 2, 2]=0, [ 3, 3]=0, A B B A B B (1) [ 1, 2]= 3, [ 1, 3]= − 2, [A2, B3]= B1, [A2, B1]= −B3, [A , B ]= B , [A , B ]= −B . 3 1 2 3 2 1 Let us consider the operators 1 1 X = i(A + iB ), Y = i(A − iB ), (2) l 2 l l l 2 l l (l =1, 2, 3). Using the relations (1), we find that
[Xk, Xl]= iεklmXm, [Yl, Ym]= iεlmnYn, [Xl, Ym]=0. (3) Further, introducing generators of the form X = X + iX , X = X − iX , + 1 2 − 1 2 (4) Y+ = Y1 + iY2, Y− = Y1 − iY2, we see that [X3, X+]= X+, [X3, X−]= −X−, [X+, X−]=2X3,
[Y3, Y+]= Y+, [Y3, Y−]= −Y−, [Y+, Y−]=2Y3. In virtue of commutativity of the relations (3) a space of an irreducible finite-dimensional repre- sentation of the group SL(2, C) can be spanned on the totality of (2l + 1)(2l˙ + 1) basis vectors | l, m; l,˙ m˙ i, where l, m, l,˙ m˙ are integer or half-integer numbers, −l ≤ m ≤ l, −l˙ ≤ m˙ ≤ l˙. Therefore,
X− | l, m; l,˙ m˙ i = (l + m)(l − m + 1) | l, m − 1, l,˙ m˙ i (m> −l), p X+ | l, m; l,˙ m˙ i = (l − m)(l + m + 1) | l, m + 1; l,˙ m˙ i (m X3 | l, m; l,˙ m˙ i = mp| l, m; l,˙ m˙ i, Y− | l, m; l,˙ m˙ i = (l˙ +m ˙ )(l˙ − m˙ + 1) | l, m; l,˙ m˙ − 1i (m> ˙ −l˙), q ˙ ˙ ˙ ˙ ˙ Y+ | l, m; l, m˙ i = (l − m˙ )(l +m ˙ + 1) | l, m; l, m˙ +1i (m< ˙ l), q ˙ ˙ Y3 | l, m; l, m˙ i =m ˙ | l, m; l, m˙ i. (5) From the relations (3) it follows that each of the sets of infinitesimal operators X and Y generates the group SU(2) and these two groups commute with each other. Thus, from the relations (3) and (5) it follows that the group SL(2, C), in essence, is equivalent locally to the group SU(2) ⊗ SU(2). 2.1 Representations of SL(2, C) As is known [12], finite-dimensional (spinor) representations of the group SO0(1, 3) in the space of symmetrical polynomials Sym(k,r) have the following form: l0−l1+1 l0+l1−1 αξ + β αξ + β Tgq(ξ, ξ)=(γξ + δ) (γξ + δ) q ; , (6) γξ + δ γξ + δ 4 where k = l0 + l1 − 1, r = l0 − l1 +1, and the pair (l0,l1) defines some representation of the group SO0(1, 3) in the Gel’fand-Naimark basis. The relation between the numbers l0, l1 and the number l (the weight of representation in the basis (5)) is given by the following formula: (l0,l1)=(l,l + 1) . Whence it immediately follows that l + l − 1 l = 0 1 . (7) 2 As is known [12], if an irreducible representation of the proper Lorentz group SO0(1, 3) is defined by the pair (l0,l1), then a conjugated representation is also irreducible and is defined by a pair ±(l0, −l1). Therefore, (l0,l1)= −l,˙ l˙ +1 . Thus, l − l +1 l˙ = 0 1 . (8) 2 Let S = sα1α2...αkα˙ 1α˙ 2...α˙ r = sα1 ⊗ sα2 ⊗···⊗ sαk ⊗ sα˙ 1 ⊗ sα˙ 2 ⊗···⊗ sα˙ r X be a spintensor polynomial, then any pair of substitutions 1 2 ... k 1 2 ... r α = , β = α1 α2 ... αk α˙ 1 α˙ 2 ... α˙ r defines a transformation (α, β) mapping S to the following polynomial: α(α1)α(α2)...α(αk)β(˙α1)β(˙α2)...β(˙αr) PαβS = s . The spintensor S is called a symmetric spintensor if at any α, β the equality PαβS = S holds. The space Sym(k,r) of symmetric spintensors has the dimensionality dim Sym(k,r) =(k + 1)(r + 1). (9) C The dimensionality of Sym(k,r) is called a degree of the representation τ ll˙ of the group SL(2, ). It is easy to see that SL(2, C) has representations of any degree. For the each A ∈ SL(2, C) we define a linear transformation of the spintensor s via the formula α˙ β˙ α˙ β˙ α˙ β˙ ˙ ˙ ˙ sα1α2...αkα˙ 1α˙ 2...α˙ r −→ Aα1β1 Aα2β2 ··· Aαkβk A 1 1 A 2 2 ··· A r r sβ1β2...βkβ1β2...βr , (βX)(β˙) ˙ ˙ ˙ ˙ where the symbols (β) and β mean β1, β2, ..., βk and β1, β2, ..., βr. This representation of SL(2, C) we denote as τ k r = τ ˙. The each irreducible finite dimensional representation of 2 , 2 ll SL(2, C) is equivalent to one from τ k/2,r/2. When the matrices A are unitary and unimodular we come to the subgroup SU(2) of SL(2, C). Irreducible representations of SU(2) are equivalent to one from the mappings A → τ k/2,0(A) with A ∈ SU(2), they are denoted as τ k/2. The representation of SU(2), obtained at the contraction A → τ k/2,r/2(A) onto A ∈ SU(2), is not irreducible. In fact, it is a direct product of τ k/2 by τ r/2, therefore, in virtue of the Clebsh-Gordan decomposition we have here a sum of representations τ k+r , τ k+r −1,..., τ k−r . 2 2 | 2 | 5 2.1.1 Definition of the spin C We claim that any irreducible finite dimensional representation τ ll˙ of the group SL(2, ) cor- responds to a particle of the spin s, where s = |l − l˙| (see also [13]). All the values of s are −s, −s +1, −s +2, ..., s or −|l − l˙|, −|l − l˙| +1, −|l − l˙| +2,..., |l − l˙|. (10) Here the numbers l and l˙ are k r l = , l˙ = , 2 2 where k and r are factor quantities in the tensor product ∗ ∗ ∗ C2 ⊗ C2 ⊗···⊗ C2 C2 ⊗ C2 ⊗···⊗ C2 (11) k times O r times | {z } | {z } ∗ associated with the representation τ k/2,r/2 of SL(2, C), where C2 and complex conjugate C2 are S biquaternion algebras. In turn, a spinspace 2k+r , associated with the tensor product (11), is S2 ⊗ S2 ⊗···⊗ S2 S˙ 2 ⊗ S˙ 2 ⊗···⊗ S˙ 2 . (12) k times O r times | {z } | {z } Usual definition of the spin we obtain at the restriction τ ll˙ → τ l,0 (or τ ll˙ → τ 0,l˙), that is, at the restriction of SL(2, C) to its subgroup SU(2). In this case the sequence of spin values (10) is reduced to −l, −l + 1, −l + 2, ..., l (or −l˙, −l˙ + 1, −l˙ + 2, ..., l˙). The products (11) and (12) define an algebraic (spinor) structure associated with the rep- resentation τ k/2,r/2 of the group SL(2, C). Usually, spinor structures are understood as double (universal) coverings of the orthogonal groups SO(p, q). For that reason it seems that the spinor structure presents itself a derivative construction. However, in accordance with Penrose twistor programme [14, 15] the spinor (twistor) structure presents a more fundamental level of reality rather then a space-time continuum. Moreover, the space-time continuum is generated by the twistor structure. This is a natural consequence of the well known fact of the van der Waerden 2-spinor formalism [16], in which any vector of the Minkowski space-time can be constructed via the pair of mutually conjugated 2-spinors. For that reason it is more adequate to consider spinors as the underlying structure1. Further, representations τ and τ ′ ′ are called interlocking irreducible representations of s1,s2 s1,s2 ′ 1 ′ 1 the Lorentz group , that is, such representations that s1 = s1 ± 2 , s2 = s2 ± 2 [20, 21]. The two most full schemes of the interlocking irreducible representations of the Lorentz group (Bhabha- Gel’fand-Yaglom chains) for integer and half-integer spins are shown on the Fig. 1 and Fig. 2. Wave equations for the fields of type (l, 0) ⊕ (0, l˙) and their solutions in the form of series in hyperspherical functions were given in [23]-[27]. It should be noted that (l, 0) ⊕ (0, l˙) type wave equations correspond to the usual definition of the spin. In turn, wave equations for the fields of type (l, l˙) ⊕ (l,l˙ ) (arbitrary spin chains) and their solutions in the form of series in generalized hyperspherical functions were studied in [28]. Wave equations for arbitrary spin chains correspond to the generalized spin s = |l − l˙|. 1 We choose Spin+(1, 3) as a generating kernel of the underlying spinor structure. However, the group Spin+(2, 4) ≃ SU(2, 2) (a universal covering of the conformal group SO0(2, 4)) can be chosen as such a kernel. The choice Spin+(2, 4) ≃ SU(2, 2) takes place in the Penrose twistor programme [15] and also in the Paneitz-Segal approach [17, 18, 19]. 6 (s,0) ... s • . . − (2,0) ... ( s+2 , s 2 ) ... 2 • 2 • 2 − (1,0) ( 3 , 1 ) ... ( s+1 , s 1 ) ... 1 • 2•2 2 • 2 (0,0) ( 1 , 1 ) (1,1) ( s , s ) s ... 2 2 ... Û 0 • 2•2 • • − (0,1) ( 1 , 3 ) ... ( s 1 , s+1 ) ... −1 • 2•2 2 • 2 − (0,2) ... ( s 2 , s+2 ) ... −2 • 2 • 2 . . (0,s) ... −s • Fig. 1: Interlocking representation scheme for the fields of integer spin (Bose-scheme), s = 0, 1, 2, 3,.... Let us consider in detail several interlocking representations (spin lines) shown on the Fig. 1 and Fig. 2. First of all, a central row (line of spin-0) in the scheme shown on the Fig. 1, 1 1 3 3 s s (0, 0) , (1, 1) , (2, 2) ··· , ··· (13) 2 2 2 2 2 2 induces a sequence of algebras ∗ ∗ ∗ ∗ ∗ ∗ C0 −→ C2 ⊗ C2 −→ C2 ⊗ C2 C2 ⊗ C2 −→ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 −→ O ∗ ∗ ∗ ∗ O −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ ... −→ O ∗ ∗ ∗ −→ C2 ⊗ C2 ⊗···⊗ C2 C2 ⊗ C2 ⊗···⊗ C2 −→ ... s times O s times | {z } | {z } 7 (s,0) ... s • . . 3 3 2s+3 2s−3 ( 2 ,0) ... ( 4 , 4 ) ... 2 • • 1 1 1 2s+1 2s−1 ( 2 ,0) (1, 2 ) ... ( 4 , 4 ) ... 2 • • • s • Û − 1 (0, 1 ) ( 1 ,1) ( 2s 1 , 2s+1 ) − 2 2 ... 4 4 ... 2 • • • − 3 (0, 3 ) ( 2s 3 , 2s+3 ) − 2 ... 4 4 ... 2 • • . . (0,s) ... −s • Fig. 2: Interlocking representation scheme for the fields of half-integer spin (Fermi-scheme), 1 3 5 s = 2 , 2 , 2 , .... Or, C0 −→ C4 −→ C8 −→ C12 −→ C16 −→ ... −→ C4s −→ ... With the spin-0 line we have a sequence of associated spinspaces S1 −→ S4 −→ S16 −→ S64 −→ S256 −→ ... −→ S22s −→ ... and also a sequence of symmetric spaces (spaces of symmetric spintensors) Sym(0,0) −→ Sym(1,1) −→ Sym(2,2) −→ Sym(3,3) −→ Sym(4,4) −→ ... −→ Sym(s,s) −→ ... Dimensionalities of Sym(s,s) (degrees of representations of Spin+(1, 3) on the spin-0 line) form a sequence 1 −→ 4 −→ 9 −→ 16 −→ 25 −→ ... On the spin-0 line (the first bosonic line) we have scalar (with positive parity P 2 = 1) and pseudoscalar (P 2 = −1) particles. Among these scalars and pseudoscalars there are particles with positive and negative charges, and also there are neutral (or truly neutral) particles. For example, the Fig. 3 shows eight pseudoscalar mesons of the spin 0, which form the octet B0 (eight- dimensional regular representation of the group SU(3)). All the particles of B0 belong to spin-0 line. 8 Strangeness Mass (MeV) ✻ K0 K+ -1 • • 496 ✁ sd su ❆ ✁ ❆ ✁ π0 ❆ π−✁ •dduu ❆ π+ 138 π -0 • ud du • ❆ •ss ✁ 549 η ❆ η ✁ ❆ ✁ ❆ us ds ✁ --1 • • 0 496 K− K Fig. 3: Octet B0 of pseudoscalar mesons with as- sociated quark structure according to SU(3)-theory. 0 (K−, K+), (K0, K ) and (π−,π+) are pairs of particles and antiparticles with respect to each other. Further, the spin-1/2 line, shown on the Fig. 2, 1 1 3 3 , 0 −→ 1, −→ , 1 −→ 2, −→ 2 2 2 2 5 2s +1 2s − 1 −→ , 2 −→ ···−→ , −→ ··· (14) 2 4 4 induces a sequence of algebras ∗ ∗ ∗ ∗ ∗ ∗ C2 −→ C2⊗C2 C2 −→ C2⊗C2⊗C2 C2⊗C2 −→ C2⊗C2⊗C2⊗C2 C2⊗C2⊗C2 −→ O O ∗ ∗ ∗ ∗ O −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ ... −→ O ∗ ∗ ∗ −→ C2 ⊗ C2 ⊗···⊗ C2 C2 ⊗ C2 ⊗···⊗ C2 −→ ... (2s+1)/2 times O (2s−1)/2 times | {z } | {z } Or, C2 −→ C6 −→ C10 −→ C14 −→ C18 −→ ... −→ C4s −→ ... With the spin-1/2 line we have a sequence of associated spinspaces S2 −→ S8 −→ S32 −→ S128 −→ S512 −→ ... −→ S22s −→ ... and also a sequence of symmetric representation spaces Sym(1,0) −→ Sym(2,1) −→ Sym(3,2) −→ −→ Sym(4,3) −→ Sym(5,4) −→ ... −→ Sym 2s+1 2s−1 −→ ... ( 2 , 2 ) with dimensions 2 −→ 6 −→ 12 −→ 20 −→ 30 −→ ... 9 On the spin-1/2 line (the first fermionic line) we have all known particles of the spin 1/2 including leptons (neutrino, electron, muon, τ-lepton, ...) and baryons. Among leptons and baryons there are particles with positive and negative charges, and also there are neutral particles. On the Fig. 4 we have the well-known supermultiplet of SU(3)-theory containing baryons of the spin 1/2 with positive parity (P 2 = 1), where a nucleon doublet (n, p) is the basic building block of the all stable matter. Strangeness Mass (MeV) ✻ n p -0 • • 939 ✁ ddu uud❆ ✁ ❆ ✁ Σ0 ❆ ❄ Σ−✁ •uds ❆ Σ+ 1192 Σ --1 • dds uus• ❆ •uds ✁ 1115 Λ ❆ Λ ✁ ❆ ✁ ❄ ❆ ssd ssu✁ --2 • • 1318 Ξ− Ξ0 Fig. 4: Octet F1/2 of baryons with associated quark structure according to SU(3)-theory. The dual spin-1/2 line 1 1 3 3 0, −→ , 1 −→ 1, −→ , 2 −→ 2 2 2 2 5 2s − 1 2s +1 −→ 2, −→ ···−→ , −→ ··· 2 4 4 induces a sequence of algebras ∗ ∗ ∗ ∗ ∗ ∗ ∗ ∗ ∗ ∗ C2 −→ C2 C2⊗C2 −→ C2⊗C2 C2⊗C2⊗C2 −→ C2⊗C2⊗C2 C2⊗C2⊗C2⊗C2 −→ O O ∗ ∗ ∗ ∗ ∗ O −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ ... −→ O ∗ ∗ ∗ −→ C2 ⊗ C2 ⊗···⊗ C2 C2 ⊗ C2 ⊗···⊗ C2 −→ ... (2s−1)/2 times O (2s+1)/2 times For the dual spin-1/2 line we have symmetric| spaces{z } | {z } Sym(0,1) −→ Sym(1,2) −→ Sym(2,3) −→ −→ Sym(3,4) −→ Sym(4,5) −→ ... −→ Sym 2s−1 2s+1 −→ ... ( 2 , 2 ) with the same dimensions and spinspaces. Further, with the spin-1 line (Fig. 1) 3 1 5 3 (1, 0) −→ , −→ (2, 1) −→ , −→ 2 2 2 2 s +1 s − 1 −→ (3, 2) −→ ···−→ , −→ ··· (15) 2 2 10 we have the underlying spinor structure generated by the following sequence of algebras: ∗ C2 ⊗ C2 −→ C2 ⊗ C2 ⊗ C2 C2 −→ O∗ ∗ ∗ ∗ ∗ −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 −→ O ∗ ∗ ∗ ∗ O −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ ... −→ O ∗ ∗ ∗ −→ C2 ⊗ C2 ⊗···⊗ C2 C2 ⊗ C2 ⊗···⊗ C2 −→ ... s+1 times O s−1 times | {z } | {z } Or, C4 −→ C8 −→ C12 −→ C16 −→ C20 −→ ... −→ C4s −→ ... With the spin-1 line we have also the following sequence of associated spinspaces S4 −→ S16 −→ S64 −→ S256 −→ S1024 −→ ... −→ S22s −→ ... In this case symmetric spaces Sym(2,0) −→ Sym(3,1) −→ Sym(4,2) −→ −→ Sym(5,3) −→ Sym(6,4) −→ ... −→ Sym(s+1,s−1) −→ ... have dimensions 3 −→ 8 −→ 15 −→ 24 −→ 35 −→ ... On the spin-1 line we have vector bosons with positive (P 2 = 1) or negative (P 2 = −1) parity. Among these bosons there are particles with positive and negative charges, and also there are neutral (or truly neutral) particles. For example, the Fig. 5 shows the octet B1 of vector mesons with negative parity. It is interesting to note that a quark structure of B1 coincides with the quark structure of the octet B0 for pseudoscalar mesons. Strangeness Mass (MeV) ✻ ∗K0 ∗K+ -1 • • 891 ✁ sd su ❆ ✁ ❆ ✁ ρ0 ❆ − ✁ •dduu ❆ ρ+ 763 ρ -0 ρ • ud du • ❆ •ss ✁ 782 ϕ ❆ ϕ ✁ ❆ ✁ ❆ us ds ✁ --1 • • 0 891 ∗K− ∗K Fig. 5: Octet B1 of vector mesons with associated quark structure according to SU(3)-theory. (∗K−, ∗K+), 0 (∗K0, ∗K ) and (ρ−, ρ+) are pairs of particles and an- tiparticles with respect to each other. 11 In turn, the dual spin-1 line 1 3 3 5 (0, 1) −→ , −→ (1, 2) −→ , −→ 2 2 2 2 s − 1 s +1 −→ (2, 3) −→ ···−→ , −→ ··· 2 2 induces the following sequence of algebras ∗ ∗ ∗ ∗ ∗ C2 ⊗ C2 −→ C2 C2 ⊗ C2 ⊗ C2 −→ O∗ ∗ ∗ ∗ ∗ ∗ ∗ ∗ ∗ −→ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ O ∗ ∗ ∗ ∗ O∗ ∗ −→ C2 ⊗ C2 ⊗ C2 ⊗ C2 C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 ⊗ C2 −→ ... −→ O ∗ ∗ ∗ −→ C2 ⊗ C2 ⊗···⊗ C2 C2 ⊗ C2 ⊗···⊗ C2 −→ ... s−1 times O s+1 times | {z } | {z } For the dual spin-1 line we have symmetric spaces Sym(0,2) −→ Sym(1,3) −→ Sym(2,4) −→ −→ Sym(3,5) −→ Sym(4,6) −→ ... −→ Sym(s−1,s+1) −→ ... with the same dimensions and spinspaces. The Fig. 1 (Bose-scheme) and Fig. 2 (Fermi-scheme) can be unified into one interlocking scheme shown on the Fig. 6. 5 5 ( 2 ,0) 2 • (2,0) ... 2 • 3 3 1 ( 2 ,0) (2, 2 ) 2 • • (1,0) ( 3 , 1 ) ... 1 • 2•2 1 1 1 3 ( 2 ,0) (1, 2 ) ( 2 ,1) 2 • • • (0,0) ( 1 , 1 ) (1,1) s ... Û 0 • 2•2 • 1 (0, 1 ) ( 1 ,1) (1, 3 ) − 2 2 2 2 • • • (0,1) ( 1 , 3 ) ... −1 • 2•2 3 (0, 3 ) ( 1 ,2) − 2 2 2 • • (0,2) ... −2 • 5 (0, 5 ) − 2 2 • 1 3 Fig. 6: Interlocking representations of the fields of any spin, s = 0, 2 , 1, 2 , .... 12 2.2 Relativistic wave equations In 1945, Bhabha [20] introduced relativistic wave equations ∂ψ iΓµ + mψ =0, µ =0, 1, 2, 3 (16) ∂xµ that describe systems with many masses and spins2. With the aim to obtain a relation between mass and spin we will find a solution of the equation (16) in the form of plane wave i(−p0x0+p1x1+p2x2+p3x3) ψ(x0, x1, x2, x3)= ψ(p0,p1,p2,p3)e . (17) Substituting the plane wave (17) into (16), we obtain (Γ0p0 − Γ1p1 − Γ2p2 − Γ3p3) ψ(p)+ mψ(p)=0. (18) Denoting Γ0p0 − Γ1p1 − Γ2p2 − Γ3p3 via Γ(p), we see from (18) that ψ(p) is an eigenvector of the matrix Γ(p) with the eigenvalue −m: Γ(p)ψ(p)= −mψ(p). (19) Let us show that a non-null solution ψ(p) of this equation exists only for the vectors p(p0,p1,p2,p3) for which the relation 2 2 2 2 2 p0 − p1 − p2 − p3 = mi 0 0 holds, where mi = µ λi, and λi are real eigenvalues of the matrix Γ0, µ is a constant. We assume that the equation (16) is finite dimensional. In this case the equation (19) admits a non-null solution for such and only such vectors p for which a determinant of the matrix Γ(p)+mE is equal to zero. Obviously, det (Γ(p)+ mE) is a polynomial on variables p0, p1, p2, p3. Denoting it via D(p0,p1,p2,p3) = D(p), we see that the polynomial D(p) is constant along the surfaces of transitivity of the Lorentz group, that is, D(p) is constant on the hyperboloids 2 2 2 2 2 s (p)= p0 − p1 − p2 − p3 = const. Hence it follows that D(p) depends only on s2(p): D(p)= D [s2(p)], where D(s2) is a polynomial on one variable s2. e e Decomposing D [s2(p)] on the factors, e2 2 2 2 2 2 2 2 2 D s (p) = c s (p) − m1 s (p) − m2 s (p) − m3 ··· s (p) − mk , (20) we see that dete (Γ(p)+ mE) is equal to zero only in the case when the vector p satisfies the condition 2 2 2 2 2 2 s (p)= p0 − p1 − p2 − p3 = mi , (21) 2 2 where mi are the roots of D. Since the numbers p0, p1, p2, p3 are real, then the roots mi should be real also. e 2 Let us find now a relation between the roots mi and eigenvalues of the matrix Γ0. Supposing 2 2 2 2 p1 = p2 = p3 = 0, we obtain s (p) = p0 and D [s (p)] = D(p0). At this point, the decomposition (20) is written as e e 2 2 2 2 2 2 2 D(p0)= c p0 − m1 p0 − m2 ··· p0 − mk =