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Gauging the conformal group

E A L O R D * and P G O S W A M I *

* Department of Applied Mathematics, ~'Dcpartment of Physics, Indian Institute of Science, Bangalore 560012, India

MS received 5 June 1985; revised 8 September 1985

Abstract. It is demonstrated that Kibble's method of gauging the Poincar6 group can be applied to the gauging of the conformal group. The action of the gauge transformations is the action ofgeneral spacetime diffeomorphisms (or coordinate transformations) combined with a local action of an I l-parameter subgroup of SO (4, 2). Because the translational subgroup is not an invariant subgroup of the con formal group the appropriate generalisation of the derivative of a physical field is not a covariant derivative in the usual sense, but this does not lead to any inconsistencies.

Keywords. Conformai group; gauge theories.

PACS No. 11"15

1. Introduction

The concept o f a gauge g r o u p has become a weU-established feature ofphysical theories, o f central importance. T h e standard method o f gauging a non-abelian internal symmetry group G is due to Yang and Mills (1954). T h e g r o u p parameters are m a d e spacetime-dependent and the covatiance o f the field equations is maintained by the introduction o f auxiliary fields, the Yang-Milis potentials or gauge potentials (they are the c o m p o n e n t s o f a connection on a principal fiber bundle with spacetime as base space and G as fiber). T h e gauging of the Poincar6 g r o u p by Kibble (1961) revealed that the gauging o f groups that act on the points o f spacetime as well as on the c o m p o n e n t s o f physical fields is a meaningful concept. The auxiliary fields in the case o f the Poincar6 group are essentially a tetrad and a metric-compatible but asymmetric linear connection on the spacetime. Taking the Lagrangian for the auxiliary fields to be the scalar curvature constructed f r o m the tetrad and connection leads to a viable extension o f Einstein's gravitational theory, now known as the ECKS (Einstein-Cartan-Kibble- Sciama) theory. An alternative Lagrangian, quadratic in curvature and torsion, also leads to a viable gravitational theory ( v o n d e r Heyde 1976; Hehl 1980; Hehl et al 1980).

The Poincar6 g r o u p is the group o f isometries o f Minkowski space. The two important candidates for extending the g r o u p are the affine g r o u p and the conformal group. Neither o f these can be an exact symmetry o f a realistic physical theory; they are to be considered as spontaneously broken symmetries. The gauging o f the affine group has been carried out by Lord (1978); there are interesting indications that the affine gauge theory may be the correct extension of Poincar6 gauge theory and could lead to an understanding o f the relationship between the gravitational and the strong interactions (Hehl et a11977, 1978). The conformal group is the fifteen-parameter g r o u p 635

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of diffeomorphisms on Minkowski space that preserves the light-cone structure. The action of this group on ordinary physical fields (representations of the Poincar~ group) can be defined, and Lagrangian theories that are invariant under conformal transform- ations can be constructed (see for example Mack and Salam 1969). The breaking of the conformal symmetry is associated with particle masses and coupling constants that are not dimensionless.

Some general principles underlying the gauging of groups of spacetime diffeomorph- isms have been worked out by Harnad and Pettitt (1976). The particular case of the conformal group was discussed by the same authors, in the language of fiber bundles and employing the concept of second order frames (Harnad and Pettitt 1977). The present work will demonstrate that the concept of second order frames is not necessary for the construction of gauge theories of the conformal group.

The approach to the gauging of the conformal group to be presented here is based on a straightforward generalisation of the method applied by Kibble to the Poincar6 group.

2. The auxiliary fields

The conformal group contains an I l-parameter subgroup H, that leaves the origin (x" = 0) fixed. It is generated by S,p (Lorentz rotations), A (dilatations) and x, (special conformal transformations) satisfying the commutation relations

[S,p,A] = 0, [s,~,~,] = ~,~p~-Kp~,,, (1)

C& K,] = K,.

Let S be a set of field components belonging to a finite-dimensional linear representa- tion of H. The infinitesimal action x" --* x" - ¢" of the conformal group on the points of Minkowski space is given by

¢" = a ~ + x # o a" + px" + 2x*c" x - c~x 2, (2) where a *, ~o ~a, p and c" are constant parameters associated respectively with translation, Lorentz rotation, dilatation and special conformal transformation; the corresponding action on the field is

,~¢ = ¢ ' a #

+ ~¢,, 1

J

= ~ daS~a + ~A + ¢~x~ 1 (3)

where di S is the substantial variation (blk = S' (x) - S (x)) and

= p + 2 c . x , J

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~,B = co,P + 2 (xPc" - x ' c p) (see, for example, Mack and Salam 1969).

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The transformation law for the derivative of ~b is

6~¢, = ~ ' ~ ¢ , + ~ i ~,¢, + ~ j ¢ + ~ . ¢ , (5)

(so long as we are discussing the global action o f the conformal group in Minkowski space, we make no distinction between Greek and Latin indices). Now,

0,¢" = a~ + pf~ + 2(c" xf~ - c~x~ - crx ~) = e~ + ~f~ (6) and

so the transformation law for the derivative can be written in the form

~ fl/ = ¢'a,~¢ + (~ + ~,~) c~,¢ + ~:d~d/ +

2(¢'S,y + ~a) ¢. (8)

We now gauge the group by allowing the parameters a', o9 "p, p and c" to be spacetime- dependent. This is equivalent to allowing ~ e ~p, ~ and ~ to become independent o f each other. The relations (6) and (7) no longer hold, so that the transformation law (5) o f the derivative does not have the form (8). We now apply the usual Yang-Mills prescription:

with the aid of auxiliary fields, we can construct a generalised derivative ¢~ which transforms with a transformation law like (8) even though the parameters are spacetime- dependent,

6~r = ¢'~,ff~ +

(~

+ ¢6~) ¢, + ]qJ~ + 2(~'S,~ + ¢~A) ~b. (9)

The generalised derivative is constructed from ~, dj~b and auxiliary fields ~ and 1~

according to

(the l~j are linear combinations of the generators o f H). The necessary transformation laws o f ~ and l~j, in order for (3) and (5) to lead to the transformation law (9) for ~ , are uniquely determined. We have

which leads to

- 4 [¢'6, + ' + a e+ [< ] ¢

+ 2(~'S,~ + ~A)~k.

The required expressions for 6 ~ and ~ 6 I~ are given by picking out the coefficients o f ~b~

and ~k. It is natural to regard the fields ~ as the components of a tetrad. Assuming the matrix (~) to be nonsingular, with inverse (e~), we have

6eJ = ~;~eJ + e,rd~ ~ - e ~ (~, + ~f~), ~ ~ (11)

~r~ = ~ o~ r'~ + r,,~j ~ + ~./~ + [~, r'~] - 2e~ ( ~ s ~ + ~A). (12) Observe that the action (3) of the gauged conformal group can be interpreted as the combined action of a general coordinate transformation (c, cr) and an 'internal' gauge group H. The auxiliary fields e~ and 1~ transform like covariant vectors under the Gcr.

Under the gauge group H, the tetrad is rotated and dilated. The final term in (12) shows that l~j is not the connection for the gauge group H. Indeed, it was already apparent from

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the presence of the final term in (9) that Ov is not a covariant derivative associated with the group H, in the usual sense--its transformation law is linear but inhomogeneous.

This is a special peculiarity o f the conformal gauge theory that is not shared by the Poincar6 gauge theory. It can be traced to the fact that the translations do not form an invariant subgroup o f the conformal group. In the following section we shall see how fully covariant Lagrangian theories can be constructed with the aid of the new derivative

~,~, in spite of the fact that this derivative does not have a homogeneous transformation law.

The transformation laws (11) and (12) can be better understood as follows. Consider a purely internal SO(4,2) symmetry generated by n~, S~p, A and r~ satisfying (1) together with

[n~,nB] = 0, [n~,Sp~] = ~ h p ~ - ~l~np, l (13)

i '

In,, A] = rt~, [n~, xp] = 2(rhpA + Sp~). J and consider the transformation law o f the connection

F~ = e~ 7t~ + F~ (14)

under the simultaneous action of a c c r and H:

6Fj = ~'t~, Fj + F;dj~' + dj~ + [~, Fj]. (15)

We find precisely the transformation laws (11) and (12) for the two parts o f Fj. Thus the tetrad and the 'pseudo-connection' l~j together constitute a connection for the group SO (4, 2).

3. Lagrangian theories

Let L (g,, dv~ ) be a Lagrangian for a theory that is invariant under the global conformal group. That is,

L = ~ 6~, + 1-1' ~d,~b = 0, (~'L), dL (16)

H' = OL/Odiq/. (17)

Employing the field equations 6L dL

- - - ~i rl' = 0, (18)

we get the Noether identities in the form

a~ ( ¢ i L - rI ~ 6¢,) = 0. (19)

The Noether currents are energy-momentum, angular momentum, the dilatation current and the special conformal current, defined as the ceoflicients of the parameters in the expression

= a O,+~co PJt'~o + p @ + c%Y'-. (20)

where

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They are, explicitly,

0~ =/_~, - IllOdj, i

~";p = x , 0 ~ - x a 0; ' + ~,B, i

~i = x,O ~, + N,

~ i = (2xax~ _ x2~,fl) 0~ + 2(x a ,ip + x=Ai) + x~

(c.f. Mack and Salam 1969), where the intrinsic currents are

¢-B = - I-VS,a¢,]

/

N = - II'a~O, ~ (22)

[

~' = - n' ~ # . . j Alternatively, observe that (16) is

O_LL fig/+ IP60iO = ~iOi L + 4~ L. (23)

0¢,

Substituting (3) and (8) into this expression gives

O.L_L ~O + Yl ~ [ ~ b + (~ + ~3~) O,~b + 2 ( ~ + ~'S,y) ~k] = 4~ L. (24) Equating coefficients of w "p, p and c" gives the following conditions for the field equations to be conformally invariant:

OL o--~ s , # + rl, (s,pa,¢ + n,, ~p¢ - n,a o,qJ) = o,

OL n , ( 1 + a)0,q, 4L, (25)

0 ~ A ¢ , + =

~L n , [ ~ , ~ # + 2(q,,A + s , , ) ¢ ] 0.

N ~.¢,+ =

When the parameters of the conformal group are made spaeetime-dependent, the covariance of the theory is lost. In fact, the change in the Lagrangian L, under the action of the group with spacetime-dependent parameters, is given by

a L = - ~ 0 0 + l-V6 ~ # = ~, (rvo¢,) OL

= c31 (~iL) - Oi (~iL - l-Pf~b).

That is,

1 ct i

3 L = c3i ( ~ i L ) - (Oia')O~ - ~ (Oio9 a),,tl, B - (dip) ~ i _ (O,¢,)9t,-i_.

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This expression is analogous to the expression given by Mukunda (1982) for the Poincar6 group. We can attempt to restore the covariance ofthe theory by replacing the derivative of~, by the generalised derivative qty. Since ¢,~ was contrived to have the same transformation law under the local action that dy~O had under the global action, it (26)

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follows that (24) and (25) will hold for the modified Lagrangian L (¢,, ~b~), if 0~¢, is replaced throughout by ~b r Hence, for the new Lagrangian,

~L 6 " OL

tSL = ~ qJ + ~ 6qJ~ = ~i O,L + 4~L (27)

(c.f. (23)). The right side is now no longer equal to O~ (~iL). A further modification o f the Lagrangian is required. We introduce an auxiliary field e and define ~ = eL so that

6£P = Oi (~'~). (28)

The required transformation law for e is

6e = c3~(~e) - 4~e. (29)

That is, e is a scalar density under a Gcrand undergoes dilation under the local action H.

An obvious prescription for e is the determinant of the tetrad,

e = le~'l. (30)

Thus, as for the Poincare group (and for internal symmetry groups), there is a simple prescription for converting a Lagrangian theory, invariant under the global conformal group, to a theory invariant under the conformal gauge group (i.e. under Gcr and the local action of H): replace derivatives by the generalised derivatives (10) and multiply by the tetrad determinant (30). Then add on a Lagrangian for the auxiliary fields--the obvious choice is

where

x / ~ go gk~ trace Fik Fj~, (31)

g,j = e~ ~ r/~ B, (32)

and

F o = 0iFj - djFi - [['i, l"j], (33)

constructed from (14) with n~, S~p, etc. belonging to the adjoint representation of SO (4,2).

References

Harnad J P and Pettitt R B 1976 J. Math. Phys. 17 1827

Harnad J P and Pettitt R B 1977 in Group theoretical methods in physics, Proc. V. Intl. Colloquium (eds) R T Sharp and B Kolman (New York: Academic Press)

Hehl F W 1980 in 6th Course of the Int. School of Cosmology and Gravitation on spin, torsion, rotation and supergrtwity (eds) P G Bergmann and V Sabbatta (New York: Plenum Press)

Hehl F W, Lord E A and Ne'eman Y 1977 Phys. Lett. BTI 432 Hehl F W, Lord E A and Ne'eman Y 1978 Phys. Rev. DI7 428

Hehl F W, Nitsch J and Von der Heyde P 1980 in general relativity andgravitation, one hundred years after the birth of Albert Einstein (ed.) A Held (New York: Plenum Press) Vol 1

Kibble T W B 1961 J. Math. Phys. 2 212 Lord E A 1978 Phys. Lett. A65 l

Mack G and Salam A 1969 Ann. Phys. 53 174

Mukunda N 1982 01 Proceedings of the Workshop on Gracitation and Relativistic Astrophysics, Ahmedabad lnd/a (eds) A Prasanna, J V Narlikar and C V Vishveshwara (Bangalore: Indian Avad. Sci.) yon der Heyde P 1976 Z. Naturforschung A31 1725

Yank C N and Mills H 1954 Phys. Reo. 96 191

References

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