Spinor Representation of Conformal Group and Gravitational Model Kohzo Nishida∗) 7 1 Department of Physics, Kyoto Sangyo University, Kyoto 603-8555, Japan 0 2 n a J 2 2 ] h p - n e g . s c i s y h Abstract p [ We consider spinor representations of the conformal group. The spacetime is 1 v constructed by the 15-dimensional vectors in the adjoint representation of SO(2,4). 4 9 On the spacetime, we construct a gravitational model that is invariant under local 1 4 transformation. 0 . 2 0 7 1 : v i X r a ∗) E-mail: [email protected] 1 typeset using PTPTEX.cls hVer.0.9i Conformal transformations play a widespread role in gravity theories.1),2),3),4) In this paper, we investigate the conformal transformations of spinors. The spinor, which describes spin-1/2particlesandantiparticles,5) containsaconsiderableamountofphysical information, making it a promising target for investigation. In addition, we construct a gravitational model that is invariant under local transformation. In general, an arbitrary 4×4 transform matrix U(x) that satisfies (γ U)† = (γ U)−1, (1) 0 0 has the generators: I, γi, iγ , iγij, γ γi. (2) 5 5 U(x) describes the conformal transformations. In fact, the following6),7) i 1 M ≡ γ , P ≡ (γ +γ γ ), ij ij i i 5 i 2 2 i 1 D ≡ γ , K ≡ (γ −γ γ ), (3) 5 i i 5 i 2 2 satisfies the conformal group [D,K ] = −iK , [D,P ] = iP i i i i [K ,P ] = 2iη D−2iM , [K ,M ] = i(η K −η K ), i j ij ij i jk ij k ik j [P ,M ] = i(η P −η P ), i jk ij k ik j [M ,M ] = i(η M +η M −η M −η M ). (4) ij kl jk il il jk ij jl jl ik Other commutators vanish. Here, we have constructed a flat tangent space at every point on the four-dimensional manifold, and we indicate the vectors in the four-dimensional tangent space by subscript Roman letters i, j, k, etc. Greek letters, such as µ and ν, are used to label four-dimensional spacetime vectors. U(x) contains within it local Lorentz transformations. Let a spinor ψ transform as ψ → ψ′ = Uψ, (5) then (3) is spinor representations of the conformal group. If we rewrite (3) as 1 1 J ≡ M , J ≡ (K −P ), J ≡ (K +P ), J ≡ D. (6) ij ij i4 i i i5 i i 54 2 2 J generates the algebra of SO(2,4): pq [J ,J ] = i(η J +η J −η J −η J ), (7) pq rs qr ps ps qr pq qs qs pr where η = (1,−1,−1,−1,1) and p,q,r,s = 0,1,···5. pq 2 U(x) can be also written as U(x) = e−iεa(x)Γa, (8) where 2Γa ≡ (γ0,γ1,γ2,γ3,iγ ,iγ01,iγ02,iγ03,iγ12,iγ13,iγ23,γ γ0,γ γ1,γ γ2,γ γ3). (9) 5 5 5 5 5 We have projected out the unit matrix I. These gamma matrices satisfy Tr(ΓaΓb) = 0 a 6= b, Tr(ΓaΓa) = 1 a = 0,8,9,10,12,13,14, Tr(ΓaΓa) = −1 a = 1,2,3,4,5,6,7,11. (10) Now, let us suppose that the spacetime transforms as the 15-dimensional vectors in the adjoint representation of SO(2,4), not the six-dimensional vectors in the fundamental rep- resentation, that is, the 15-dimensional coordinates x (a = 0,1,···14) transform as a X → X′ = U−1XU, X ≡ x Γa. (11) a Notethatγ U withthegenerators(2)isthetransformmatrixofU(4). Thespacecoordinates 0 are rotated in the adjoint representation of SU(2). Therefore, it is not unnatural that the spacetime transforms in the adjoint representation. An invariant can be constructed: Tr(XX) = x2 −x2 −x2 −x2 −x2 −x2 −x2 −x2 0 1 2 3 4 5 6 7 +x2 +x2 +x2 −x2 +x2 +x2 +x2 . (12) 8 9 10 11 12 13 14 Then, themetricofthetangentspaceisη = (1,−1,−1,−1,−1,−1,−1,−1,1,1,1,−1,1,1,1). ab Let us define a 15-dimensional tetrad eaαe β = gαβ, ea ebα = ηab, (13) a α where indices a,b,c are 15-dimensional vectors in flat space and α,β,γ are 15-dimensional vectors in curved space. The 15-dimensional tetrad transforms linearly as e α(x)Γa → U−1(x)Γα(x)U(x) = e α(x)U−1(x)ΓaU(x) = e′ α(x′)Γa. (14) a a a Next, we propose a gauge model on this spacetime. In our previous paper,8) we have considered the four- and five-dimensional gauge model. The covariant derivative is given by D ≡ ∂ −igA , A ≡ A Γa, (15) α α α α aα 3 where we introduce gauge fields A , each transforming as α 1 A → A′ = UA U−1 + U∂ U−1. (16) α α α ig α The covariant derivative transforms as D → D′ = UD U−1. (17) α α α In general, the covariant derivative of the tetrad should be zero:9) ∂ e +gω ej −Γλ e = 0, (18) µ iν ij,µ ν νµ iλ where Γλ is the Christoffel symbol and ω is the spin connection. (18) can be rewritten νµ ij,µ as [D ,γ ] = Γλ γ , (19) µ ν νµ λ where i D ≡ ∂ +gω , ω ≡ ω γij. (20) µ µ µ µ ij,µ 4 In direct analogy, we require [D ,Γ ] = Γγ Γ . (21) α β βα γ Using this, we can calculate [[D ,D ],Γ ] as α β γ [[D ,D ],Γ ] = [D ,[D ,Γ ]]−[D ,[D ,Γ ]] α β γ α β γ β α γ = {∂ Γδ +Γδ Γǫ −(α ↔ β)}Γ α γβ ǫα γβ δ = R(15)δ Γ , (22) γ,αβ δ where R(15)δ ≡ ∂ Γδ −∂ Γδ +Γδ Γǫ −Γδ Γǫ is the 15-dimensional Riemann γ,αβ α γβ β γα ǫα γβ ǫβ γα curvature tensor. We multiply both sides of (22) by Γ and consider the trace to obtain ζ 1 R(15) = −2Tr(Γ [D ,D ]), Γαβ ≡ [Γα,Γβ]. (23) γδ,αβ γδ α β 2 Therefore, the 15-dimensional Riemann curvature tensor is invariant under the transforma- tion of U(x). Let us now try to form an action with this formalism. We find that the following La- grangian 1 L = e ψ¯(2iΓ Dα −m)ψ + R(15) (24) α (cid:26) 16πG(15) (cid:27) is invariant under the transformation of U(x), where R(15) is the 15-dimensional Ricci cur- vature and G(15) is the 15-dimensional constant of gravitation. The Dirac’s equation is (2iΓa∂ −m)ψ = 0. (25) a 4 On multiplying (25) by 2Γb∂ from the left, we obtain the high-dimensional Klein–Cordon b equation: (∂ ∂i −∂(5)∂(5) +∂ ∂ij −∂(5)∂(5)i −iεijklγ ∂ ∂ i ij i 5 ij kl +2iγij∂(5)∂ −2iεijklγ ∂ ∂(5) −2iεijklγ ∂(5)∂ ij kl i j kl ij −2εijklγ γ ∂ ∂ +2iεijklγ ∂ ∂(5))ψ +m2ψ = 0, (26) 5 l i jk k ij k where the summation of ∂ are limited to i < j and we represent the 15-dimensional coor- ij dinates corresponding to (9) as xa = (x0,x1,x2,x3,x(5),x01,x02,x03,x12,x13,x23,x(5)0,x(5)1,x(5)2,x(5)3). (27) Our model still cannot explain why the conformal symmetry is broken. However, it is interesting that the extra dimension and the four-dimensions have a different spatial structures compared with common high-dimensional models. Through conformal symmetry breaking, our model would undergo the reduction from 15 down to four dimensions, and the gauge-fixed tetrad must be eiµe ν = gµν ei ejµ = ηij, i,j,µ,ν = 0,2,3,4. (28) i µ Note that the following tetrad also constructs four-dimensional spacetime: eiµe ν = gµν ei ejµ = ηij, i,j = 11,12,13,14, µ,ν = 0,2,3,4. (29) i µ This would seem to suggest that there is a new internal degree of freedom in our spacetime. References 1) H. Weyl, Annalen Phys. 59, 101 (1919). 2) P. Di Francesco, P. Mathieu and D. Senechal, Conformal Field Theory (Springer, New York, 1997). 3) Y. Fujii and K. Maeda, The Scalar-Tensor Theory of Gravitation (Cambridge Univer- sity Press, Cambridge, 2003). 4) A. Jakubiec, J. Kijowski, Gen. Rel. Grav. 19, 719 (1987). 5) P.A.M. Dirac, Annuals of Mathematics 37, 429 (1936). 6) L. YuFen, M. ZhongQi, and H. BoYuan, Commun. Theor. Phys. 31, 481 (1999)[arXiv:9907009 [hep-th]]. 7) R. Shurtleff, arXiv:1607.01250v1[gen-ph]. 8) K. Nishida, Prog. Theor. Phys. 123, 227 (2010)[arXiv:1207.0211[hep-th]]. 9) R. Utiyama, Phys. Rev. 101 (1956), 1597 5