Readings on scale, conformal and Weyl invariance

 

This is a subject that has given rise to much misunderstanding, because the same words are often used by different authors to mean subtly different things. This page contains a list of papers on scale, conformal and Weyl invariance, with comments. By reviewing these papers I have tried to clarify for myself the source of many misunderstandings and establish a set of conventions that is ambiguity-free. I hope it may be useful to others too.


Preliminary mathematical notions.
Two metric tensors g and g' are said to be conformally related if g'=
Ω2 g for some nowhere vanishing function Omega. This is equivalent to the condition that the angles between any two vectors measured with the metrics g and g' are the same.
A diffeomorphism of a manifold
is said to be an isometry if the pullback of the metric g is equal to g, and a conformal transformation if the pullback of g is conformally related to g.

The isometries of a Riemannian manifold form a Lie group (the isometry group) whose Lie algebra consists of the Killing vectorfields, i.e. the vectorfields along which the Lie derivative of the metric is zero. The conformal transformations of a Riemannian manifold form a group called the conformal group, whose Lie algebra consists of the conformal Killing vectorfields, i.e. the vectorfields along which the Lie derivative of the metric is proportional to the metric.
The isometry group of Minkowski space is the Poincare' group (the semidirect product of translations and SO(1,3)) and the conformal isometries form the group SO(2,4). Most Riemannian manifolds do not have any conformal Killing vectors, so their conformal group is trivial (a fortiori their isometry group is trivial).
The term "conformal group" is sometimes also used in another sense, namely as the infinite dimensional abelian group of all conformal rescalings of a metric. This is not a group of transformations acting on spacetime; it is instead akin to the infinite dimensional group of gauge transformations in a gauge theory.


            -----------------------------------------


E. Cunningham, Proc, London Math. Soc. 8, 77 (1909)
H. Bateman,
Proc, London Math. Soc. 8, 223 (1910)

These papers are listed here for historical reasons. They showed that Maxwell's equations are covariant under the 15-parameter conformal group, and are probably the first reference to this group in the physical literature.


H. Weyl, Gravitation und Elektrizität
Sitzungsber. der K. Preuss. Akad der Wiss. zu Berlin 465,(1918)

Any review of this subject must start from Weyl's classic paper. Its main focus is the unification of gravity and electromagnetism, which I have briefly discussed elsewhere, but here we are more interested in his critique of Einstein's theory. Weyl observes that in Riemannian geometry parallel transport is generally not integrable, so that two vectors at two different points cannot be compared. However, Riemannian parallel transport preserves the length of vectors, so the length of two vectors at two different points can be compared. Why should the direction of a vector have no absolute meaning, but its length have one? This, he says, "has no factual basis, and only seems to be due to the derivation of the theory from the flat one". For Weyl, this fact goes against the idea of an "infinitesimal geometry", where only infinitesimally close vectors can be compared. In modern geometrical language, Weyl advocates dropping the assumption that the connection is metric (i.e. the covariant derivative of the metric vanishes). The theory must then be invariant not just under coordinate transformations, but also under conformal rescalings of the metric.


In an appendix to the paper, Einstein points out that if the metric properties of a spacetime could only be determined by use of light rays, then indeed the metric could only be determined up to an unknown function. But in practice we have at our disposal (infinitesimal) rigid rods and clocks, which can be used to define the line element ds. This definition of ds would only be illusory if the notions of unit length and unit time depended on the previous history of the rods and clocks. This seems not to be the case, so, he concludes, the basic assumption of Weyl's theory is false. There are counterarguments by Weyl, but it is clear that Einstein has a more profound grasp of empirical reality. Weyl admits that he may be on the wrong track (he uses the wonderful expression "auf dem Holzwege sein", which stems from the fact that paths used to carry logs out of a forest do not lead anywhere). In a note added in 1955 he admits that his attempt was misplaced and that the proper setting for the gauge invariance of electromagnetism is the phase of the quantum wave function of charged particles and not the scale.


It is important to realize that while the physical interpretation of Weyl's theory was certainly wrong, this does not rule it out: it is sufficient to reinterpret Weyl's potential as a different gauge field. Then, Einstein's objection would not apply: the fact that atoms all have the same size and energy levels just tells us that in the spacetime region where atoms existed, the curvature of this connection was zero. An extension of this argument to protons would push the statement back to before baryogenesis. In most conceivable models (see below) the Weyl gauge field would probably have a Planck-size mass and this restriction could be easily accommodated.


We now fast forward by more than forty years and consider the following famous work:


Brans and R.H. Dicke,
Mach's principle and a relativistic theory of gravitation

Phys. Rev. 124, 925 (1961)

R.H. Dicke,
Mach's principle and invariance under transformations of units
Phys. Rev. 126, 2163 (1962)

These two papers were motivated by the desire to formulate a theory of gravity that incorporates Mach's ideas on the origin of inertia. This motivation has been largely forgotten and the work is important because it is one of the first instances of what we now call scalar-tensor theories of gravity. They are also admirable examples of clear physical thinking. The authors are careful to define the theory in ways that have operational meaning, and in so doing they find themselves echoing Weyl's call for a "truly infinitesimal geometry". In the first paper they say that "there is no direct way in which the mass of a particle...can be compared with that of another at a different space-time point". And in the second Dicke adds: "It is evident that two rods side by side, stationary with respect to each other, can be intercompared....this cannot be done for....rods with either a space- or time-like separation". There follows that a statement such as "a hydrogen atom on Sirius has the same diameter as one on the Earth...is either a definition or else meaningless". The resulting local arbitrariness in the choice of units reflects itself in the definition of the metric: different choices of units lead to metrics that are conformally related. This does not mean that Riemannian geometry is useless or incorrect, just that each Riemannian geometry is a particular representation of the theory. The physical content of the theory should be contained in the invariants of position dependent transformations of units and coordinate transformations. In general relativity the representation is one in which units are chosen so that atoms are described as having physical properties independent of location. That such a representation exists is in itself a nontrivial assumption.


In Brans and Dicke's theory, it is assumed that all mass ratios of elementary particles are constant. In the first paper a system of units is chosen such that the masses are themselves constant throughout spacetime. Then, Newton's constant is allowed to be position dependent and is treated as a field. The Lagrangian of Brans-Dicke theory in these units consists of a kinetic term for the scalar, coupled nonminimally to the curvature scalar. The matter Lagrangian is assumed to depend on the metric but not on the scalar, in such a way that the equations of motion of matter in a given background geometry are the same as in general relativity. In the second paper the same theory is discussed in the system of units where Newton's constant is assumed to be constant and the particle masses are allowed to depend on position. This reformulation differs from the previous one by a conformal transformation. In the new "conformal frame" the equations for the metric are the same as in Einstein's theory, but matter now couples to the scalar, which can be seen as another matter field. It is important to note that the Brans-Dicke action is not Weyl-invariant (except for the special choice of parameter -3/2).


P.A.M. Dirac,
Long range forces and broken symmetries
Proc. Roy. Soc. 333, 403 (1973)

Dirac, like many others, was fascinated by Weyl's theory, which he describes as "the outstanding [unified theory], unrivalled by its simplicity and beauty", Yet, it clashes with quantum theory: "quantum phenomena provide an absolute standard of length...[and] there is no need for the arbitrary metric standards of Weyl's theory". In this late paper Dirac tries to resuscitate Weyl's theory. He starts from the "large number hypothesis" that he had formulated in 1938. It is a speculation that all the very large dimensionless numbers that one can form are related by some as yet unknown law, and it leads to the conclusion that Newton's constant has to decrease in proportion to the age of the universe. Assuming that this hypothesis is correct, the question is how to reconcile it with Einstein's theory of gravitation, which requires that G shall be constant. Dirac's suggestion is that "the Einstein equations refer to an interval dsE connecting two neighboring points that is not the same as the interval dsA measured by atomic apparatus. By taking the ratio of dsE to dsA to vary with the epoch we get G varying with the epoch".
"With the introduction of the two metrices
dsE and dsA we see that the objection to Weyl's theory...falls away. One can apply Weyl's geometry to dsE, supposing it is nonintegrable when transported by parallel displacement, so that we must refer to an arbitrary metric gauge to get a definite value for it...On the other hand dsA is referred to atomic units and is not affected by a [conformal] transformation..."

"The measurements ordinarily made by physicists in the laboratory use apparatus which is fixed by the atomic properties of matter, so the measurements will refer to the metric dsA. The metric dsE cannot be measured directly, but it shows itself up through the equations of motion.... The relation of the two metrics is exemplified by radar observations of the planets. Here a distance which is determined by equations of motion is measured by atomic apparatus."

Dirac then goes on to review the formalism of Weyl geometry and proposes a Lagrangian which is essentially the same as the one of Brans and Dicke. Perhaps the most original part of the paper is the prediction that in this theory there will be C and T violating effects, with CT preserved. Unfortunately this conclusion only applies when the Weyl gauge field is interpreted as the electromagnetic potential. In the conclusions Dirac asks why one should believe in such a theory. Even if the variation of G was confirmed by experiment, it would not prove that Weyl's geometry is needed to explain the electromagnetic field. Dirac says that "it appears as one of the fundamental principles of Nature that the equations expressing basic laws should be invariant under the widest possible group of transformations... The passage to Weyl's geometry is a further step in the direction of widening the group of tranformations underlying physical laws."


I have listed this paper here because it makes a clear case for the existence of different spacetime metrics, related to different fundamental units. However, this notion had been discussed earlier in the literature and Dirac's insistence on Weyl's original interpretation is clearly misplaced. Furthermore, some of its conclusions are incorrect, as pointed out in the following paper.


J. Bekenstein and A. Meisels
Conformal invariance, microscopic physics and the nature of gravitation
Phys. Rev. D22, 1313-1324 (1980)

The focus of this paper is the question whether the gravitational constant could be spacetime dependent. Starting from the observation that physical laws are invariant under global rescalings of the units of length, and the axiom that this invariance should be extended to local rescalings, it is observed that this would also imply that all Compton wavelength should be allowed to transform, and therefore all particle masses should become scalar fields. For the theory to be complete, it must prescribe a dynamics for each such mass field. The authors assume that all mass ratios are constant and therefore all masses are proportional to a single mass field. From a set of postulates, including Weyl invariance, the action of the mass field is derived to be that of a conformally coupled scalar, plus a quartic potential. This theory is known to be equivalent to Einstein's theory in the frame where the mass field is contant. But the authors point out that "this conclusion...is an understantement. The physical content of the theory is the same in any units. It is GR in any conformal frame." The ratio of Newton's constant to any particle mass is constant. The conclusion is that the "the simplest implementation of the principle of conformal invariance requires that gravitation be described by GR" with Newton's constant a constant when measured in particle masses.


There is then a sharp criticism of Dirac's preceding paper, and other attempts to introduce a variable Newton's constant. Regarding Dirac's paper they observe that the proposed action for a pointlike particle is the integral of the line element including a factor of the universal mass field, and a constant dimensionless prefactor. This action is Weyl invariant. Dirac defines Einstein units to be those where the mass field is constant. He regards these as distinct from atomic units. "Yet the particular theory at hand fails to incorporate this distinction". In fact, in the Einstein frame particle masses as defined above are also constant. "Thus, despite his avowed intention to write a theory which distingushes between Einstein and atomic units, the theory at hand does not do this... it is evidently GR in a conformally invariant garb.... The failure to incorporate a distinction between the units can be traced to the use of a single field... to describe the characteristic length associated with gravitation, and that associated with rest masses."


E.E. Flanagan,
The conformal frame freedom in theories of gravitation

Class. and Quantum Grav. 21, 3817 (2004)

arXiv gr-qc/0403063

This paper contains a clear discussion of the issue of the choice of conformal frame. The issue can be stated as follows: suppose we are given two Lagrangians for gravity and matter, which can be obtained from each other by means of a Weyl redefinition of the metric. Should the two theories be regarded as physically equivalent? The answer to this question depends on the physical interpretation of the metric in the two frames, and a lot of confusion has been generated in the literature by the fact that authors often fail to state such assumptions explicitly. If one assumes that the metric in both theories is the metric measured by means of atomic clocks, then indeed the two theories will be physically inequivalent. However, if one sticks to the interpretation mentioned above that conformal redefinitions of the metric simply amount to different choices of units, then the two theories must be physically equivalent. This interpretation is by far the most natural and attractive one, as it agrees fully with the notion that a choice of conformal frame is a choice of gauge, and is therefore in line with the terminology that has developed historically since Weyl's original paper.

The discussion is a little less complete in the quantum case, which will be discussed below. It is pointed out, however, that if the theory is treated as an effective quantum field theory, then applying a standard result, physical observables (more precisely: the S matrix) do not change under field redefinitions, so also in this context two theories that differ by a conformal redefinition of the metric must be equivalent.


A. Iorio, L. O'Raifeartaigh, I. Sachs and C. Wiesendanger
Weyl gauging and conformal invariance

Nucl. Phys. B495, 433-450 (1997)

arXiv:hep-th/9607110
This article explores the relation between conformal invariance (in flat spacetime) and Weyl invariance (in curved spacetime). Starting from rigid transformations on flat space, it is clear that rescalings of the coordinates and rescalings of the metric are physically equivalent. In curved space, a theory that is rigid Weyl invariant can be made local Weyl invariant by introducing a gauge potential. This is called "Weyl gauging" (when the Weyl gauge potential is flat, it can be traded for a dilaton). In some cases the theory can be made locally Weyl invariant without having to introduce a gauge field, just by introducing suitable couplings to the Ricci tensor. This is called "Ricci gauging". It is shown that if a theory is conformally invariant in flat space, ita admits Ricci gauging. The converse is also true for Lagrangians that depend at most on first derivatives of the fields. Conformally invariant Lagrangians for fields of any spin are given.


We now go over to the context of quantum field theory. The first few papers listed below discuss mostly some results regarding conformal invariance in flat space (i.e. invariance under the conformal group SO(2,d)).


C.G. Callan, S. Coleman and R. Jackiw,
A new improved energy-momentum tensor

Ann. of Phys. 59, 42 (1970)

S. Deser,
Scale invariance and gravitational coupling

Ann. of Phys. 59, 248 (1970)

In a renormalizable theory, the matrix elements of the energy-momentum tensor at zero momentum are finite, because they are related to the total energy and momentum of the system. Likewise, the first derivatives at zero momentum are finite because they are related to the Lorentz generators. Not much can be said a priori about higher derivatives. Still, the energy-momentum tensor is an important observable that enters in the scattering amplitudes in an external gravitational field, and one would like them to be finite too. 
In the classic paper by CCJ it is shown that the canonical energy momentum tensor (and even its symmetric improvement, due to Belinfante) do not always satisfy this requirement. However, in a renormalizable theory it is possible to define a "new improved" energy momentum tensor that upon integration gives the same values of the energy and momentum but is always finite. It is then shown that this is the same tensor that one would define by requiring that the divergence of the scale current take a particularly simple form.
When the new improved energy momentum tensor is coupled to a transverse traceless graviton, the improvement terms vanish. However, this is not true when it couples to an external gravitational field. The scattering amplitude is finite with the new improved tensor, whereas it would diverge with the conventional energy-momentum tensor. Finally, one can ask what modification would be needed in the gravitational Lagrangian so that the new improved energy-momentum tensor acted as the source of gravity. In the case of the scalar field, the answer is a nonminimal coupling
Φ2R/12.

Deser comes to similar conclusions, from a slightly different direction. He observes that the energy-momentum tensor of a massless scalar can be made traceless by adding, by hand, a suitable "improvement" term. This term can be seen, from a more fundamental point of view, as coming from a nonminimal interaction term in the Lagrangian. Then he observes that the equation of motion for the metric deriving from this action is very similar to Einstein's equations coupled to the improved scalar energy-momentum tensor, except that "Newton's constant", which is now proportional to -6 times the inverse square of the scalar, now has the wrong sign for the gravitons to have positive energy. Deser suggests taking this action, with the overall sign changed, as a basis for a theory of gravitation. It is observed that in order to couple consistently to this theory, any other matter must have a traceless energy-momentum tensor (on shell). Breaking of scale invariance by a potential is also discussed.
A terminological note: Deser's paper begins with the statement that "Scale invariance of a material system....means that it does not involve dimensional parameters". It is clear that the scale invariance considered here is not the one that Weyl or Brans and Dicke had in mind. For Deser, as for most particle physicists, a system is (either globally or locally) scale invariant when the action is invariant under rescalings of the fields, but not of the other parameters of the theory such as masses and couplings. Weyl and most general relativists consider instead transformations acting on all the quantities appearing in a theory, including masses and couplings.


S. Coleman and R. Jackiw,
Why dilatation generators do not generate dilatations?

Ann. of Phys. 67, 552 (1971)

The motivation for this work comes from the idea that at high energy masses become negligible and therefore a theory should become approximately scale invariant, in some suitable sense. The context of this work are power counting renormalizable theories (i.e. theories with dimensionless coupling constants). Then it appears that the only possible source of breaking of scale invariance are mass terms. If one applies standard canonical methods, one can construct a current that generates dilatations and derive from it theorems about the asymptotic behavior of Green functions. These theorems are false in perturbation theory. The reason is that the formal manipulations leading to them do not go through when one introduces a cutoff. This is simple to understand: a large cutoff is a large dimensionful scale in the theory, and it leaves behind a residue called a scale anomaly.


The main results of the paper are: (1) in lowest order of perturbation theory, the scale anomaly can be completely described by a change in the scale dimension of the field, (2) at higher orders, the anomaly cannot be explained simply by a change of the scale dimension. The authors stress the difference between the notion of scale dimension and the usual notion of dimension as used in dimensional analysis. In both cases the dimension is the power of the scaling parameter that must multiply a field in order to preserve scale invariance. But "the transformations of dimensional analysis map the exact solutions of one field theory into the exact solutions of a different field theory, with different masses. Scale transformations... stay within a given field theory, and do not map solutions into solutions, unless the masses are zero". This is an important difference between the notion of scale (or Weyl) invariance as commonly used by particle physicists and general relativists.


S. Coleman

Dilatations

lectures given in Erice (1971)
published in "Properties of the fundamental interactions",
Editrice Compositori, Bologna (1973)
reprinted in "Aspects of symmetry",
Cambridge University Press (1985)

In these lecture notes Coleman discusses, with his customary clarity, the status of dilatation and conformal invariance in quantum field theory. He starts from the formal Ward identities that follow from dilatation invariance, and the low energy theorems that follow from them, emphasizing the analogy to chiral symmetry and current algebra. He then gives an argument showing that these theorems must be violated in the deep euclidean region. The reason for the violation are "anomalies". One such "anomaly" is the anomalous dimension discussed in the preceding paper. He says "it would be very pleasant if...all anomalies could be absorbed into a redefinition of the scale dimension.... this is not what happens". Fortunately, at least in a renormalizable theory, it turns out that there is just one other type of "anomaly", namely the scale dependence of coupling constants, described by the beta functions. The correct equations that replace the false low energy theorems is the Callan-Symanzik (CS) equation. Says Coleman: "Unlike the low energy theorems of current algebra, which they so closely resemble, the CS equations are practically useless for low energy phenomenology. It is the beta terms that make the difference. A current algebra low energy theorem is useful because it expresses one Green's function in terms of another in a way that does not depend on strong interaction dynamics. The CS equations, on the other hand, expresses one Green's function in terms of another and its derivatives with respect to coupling constants. If you know how to compute these, you have already solved the strong interaction dynamics and there is no reason for you to be piddling around with low energy theorems".

However, in the deep euclidean region the Callan-Symanzik equation simplifies and becomes the renormalization group equation of Gell-Mann and Low. Coleman gives an independent, alternative argument for this equation and says "This argument seems to me to owe very little to asymptotic estimates derived from perturbation theory... therefore I will assume...that the renormalization group equations are valid independent of perturbation theory". These equations imply that the asymptotic form of Green's functions in the deep euclidean region can be expressed as a function of a "running coupling", itself a function of the coupling and a momentum scale, which is obtained by solving a first order differential equation. "This is useful information as it stands; for example it has been used to enormously simplify the summation of leading logarithms. However, as was pointed out by Wilson, if we make some (apparently very mild) additional assumptions, we get a surprisingly greater amount of information". The additional assumptions are continuity of the functions appearing in the RG equation, and the existence of a zero of the beta function with negative derivative. Under these assumptions, the running coupling will flow towards the zero at high energy and Green's functions will again display scaling, with the only anomalies being anomalous dimensions. "The beta anomalies, which complicate things terribly at low energies, simplify things enormously in the deep euclidean region. What a wonderful reversal!"

J. Polchinski,
Scale and conformal invariance in quantum field theory

Nucl. Phys. B303, 226 (1988)

R. Jackiw and S.-Y. Pi,
Tutorial on scale and conformal symmetries in diverse dimensions,
J. Phys. A44, 223001 (2011)

arXiv:1101.4886 [math-ph]

S. El-Showk, Y. Nakayama, S. Rychkov,
What Maxwell theory in d\not=4 teaches us about scale and conformal invariance

Nucl. Phys. B848, 578 (2011)

arXiv:1101:5385 [hep-th]
These three papers are concerned with the following issue: under what conditions does invariance under Poincare and scale transformations imply invariance under special conformal transformations (and hence under the whole SO(2,d))? (The converse statement, namely Poincare and special conformal invariance implying scale invariance, is always true just for Lie algebraic reasons.) It is sometimes erroneously assumed that the implication is always true. Polchinski gives several examples of theories that are scale invariant and not conformally invariant, but such examples are all somewhat pathological. He then proves (completing an argument by Zamolodchikov) that in two dimensions for every unitary theory having a discrete spectrum of operator dimensions, scale invariance implies conformal invariance. The question remained open whether the same statement also holds in higher dimensions.
The other two papers provide a simple counterexample: Maxwell theory in five dimensions.



Now we come to Weyl transformations and we begin by discussing quantum fields in a background geometry. The most important new phenomenon that we have to take into account is the conformal anomaly. This can be stated as follows. Suppose the classical action of the system S(g,Φ) is invariant under Weyl transformations: S(Ω2g,Ω-dΦ)=S(g,Φ), where d is the length dimension of the field Φ. (Note that even though we treat the background as fixed, we allow coordinate transformations and Weyl transformations to act on it. This means that we are not treating the metric g as a fixed background, but rather its diffeomorphism equivalence class and, in the conformal invariant case, its Weyl equivalence class.) Next we compute the effective action Γ(g,Φ). Many different calculations lead to the conclusion that even though the classical action is invariant under Weyl transformations, the effective action is not. Before discussing this in greater detail let me first quote some classic papers on the subject:


D.M. Capper and M.J. Duff,
Trace anomalies in dimensional regularization

Nuovo Cim. A23,173 (1974)
Conformal anomalies and the renormalizability problem in quantum gravity
Phys. Lett.A53, 361 (1975)

The reason for the existence of the conformal anomaly can be understood by observing that even when a theory is scale invariant and hence contains no dimensionful couplings, the definition of the quantum theory always involves some mass scale (for example a cutoff or a renormalization scale; in dimensional regularization a mass has to be introduced to preserve the proper canonical dimensions; in zeta function regularization one encounters the sums of powers of eigenvalues or logarithms of eigenvalues, both requiring an external reference mass in order to make dimensional sense). Then, the renormalized theory carries some trace of this mass scale, thus breaking scale invariance.

F. Englert, C. Truffin and R. Gastmans,
Conformal invariance in quantum gravity

Nucl. Phys. B117, 407 (1976)
Apparently in contradiction to the previous two papers, and many others that rederived the anomaly in a variety of ways, the authors of this paper claim that it is possible to carry over Weyl invariance from the classical to the quantum theory. The important caveat is that this is possible if conformal invariance is spontaneously broken, which is a way of saying that there exists a dilaton field. The proof is based on the fact that by inserting suitable powers of the dilaton in the action, one can dimensionally continue the theory always preserving conformal invariance. This theory, being invariant in all dimensions, remains invariant after divergences are removed by suitable counterterms. The result is that there is no anomaly.

The contradiction between this result and the previous ones is only apparent. In reality, the starting theories are quite different. The theories where an anomaly appears are special theories that contain no dimensionful parameters. On the other hand suppose one starts from a completely arbitrary theory and splits the metric into g=
Φ2 ĝ, where Φ is a scalar field called the dilaton. Then the action is automatically invariant under the "split symmetry" ĝ-->Ω2ĝΦ-->Ω-1Φ. This is completely analogous to Stückelberg's treatment of massive QED, which can be made gauge invariant by introducing a phase-valued scalar field. It is this field Φ that Englert et al use to dimensionally regularize the theory in a Weyl invariant way. Without it, this is not possible and the anomaly appears.

The story of the conformal anomaly is told with much wit and detail by one of its main characters in:

M.J. Duff,
Twenty years of the Weyl anomaly
talk given at the Salamfest - Trieste 1993
Class. and Quantum Grav. 11, 1387 (1994)
arXiv:hep-th/9308075

Before we go on with other ideas it is worthwile to observe that the result of Englert et al, though derived in the context of dimensional regularization, is much more general. Incidentally, my view on this issue has been explained in the following two papers:

R.Floreanini and R. Percacci,
Average effective potential for the conformal factor
Nucl. Phys. B436, 141 (1995)
arXiv: hep-th/9305172
Renormalization group flow of the dilaton potential
Phys. Rev. D52, 896 (1995)
arXiv: hep-th/9412181
These papers introduce the split symmetry and the associated dilaton, here regarded as the conformal factor of the metric, in a theory of gravity with independent metric and connection. The details of the model are not especially important for our discussion. The aim of the papers was to calculate the effective potential of the dilaton. A momentum cutoff regularization is used, and it is observed that in defining this cutoff one has a choice: the norm of the momentum can be defined either with the original metric g or with the split metric ĝ. In the former case, the cutoff is defined in a way that respects the split symmetry and as a result one finds that also the effective action is invariant, and thus can be written as a function of the original metric g only. In this case the only possible potential is Φ4, which in terms of g corresponds to a cosmological term. In the latter case the cutoff introduces in the quantum theory a dependence on the metric ĝ which is not accompanied by a suitable power of the dilaton, and therefore breaks the split symmetry. In this case, which was the main focus of these papers, the effective action is a function of ĝ and Φ separately and a nontrivial effective potential for Φ is generated quantum mechanically.

The following recent paper explains how to preserve local scale invariance in lattice regularization, in the presence of a dilaton:

M. Shaposhnikov and I. Tkachev,
Quantum scale invariance on the lattice
Phys. Lett. B675, 403 (2009)

arXiv:0811.1967 [hep-th]

The observation by Deser that a conformally coupled theory can be taken as a basis for a theory of gravity has given rise to a large literature. A few of these papers are reviewed below.

A. Zee,
Broken-Symmetric theory of gravity

Phys. Rev. Lett. 42, 417 (1979)

This is one of the first papers that over the years made similar proposals. Zee starts by comparing Einstein's theory of gravity to Fermi's theory of the weak interactions: both are nonrenormalizable. In the standard model, Fermi's coupling constant is identified with the inverse square of the VEV of a scalar field. Perhaps by thinking also of Newton's constant as the VEV of a scalar one can relate the weakness of gravity to the massiveness of some particle. The Lagrangian proposed by Zee has a single scalar field with a potential and interacting with gravity via a nonminimal term Φ2R. The potential is assumed to have the usual shape that induces a nonzero VEV for the scalar. This VEV is then related to Newton's constant and the scalar field has a mass of the order of the Planck mass. In analyzing the equations of motion of the theory, Zee demands that the exchange of energy between matter and the gravitational field be described exactly as in Einstein's theory. He shows that this is the case provided the Lagrangian for other matter fields does not depend on the scalar. On the other hand, the large value of the VEV suggests that there may be a relation between the scalar generating Newton's constant and the Higgs field breaking GUT. If this is true, then the matter Lagrangian also depends on the scalar. Conservation of the matter energy-momentum tensor follows only in a region where the scalar is constant, such as here and now.

Says Zee: "The concept of spontaneous symmetry breakdown has proven extraordinarily fruitful in many areas of physics and I consider it worthwile to try to incorporate it into a theory of gravitation". If one is reading this paper together with the other ones listed here, it is easy to think that Zee has in mind spontaneous breaking of scale or conformal invariance. But this is not the case. In fact scale invariance is not mentioned even once. It is true that in Zee's model scale invariance is broken, but it is broken explicitly by the potential. So, while the paper is formally correct, I find the insistence on the notion of spontaneous symmetry breaking somewhat misleading, because no symmetry is being spontaneously broken (unless one wants to think of the scalar as the Higgs of SU(5), but that really is optional and has nothing to do with gravity).

W. Buchmüller and N. Dragon,
Scale invariance and spontaneous symmetry breaking,
Phys. Lett. B195, 417-422 (1987)
Dilatons in flat and curved space-time
Nucl. Phys. B321, 207-231 (1989)
These papers start from the observation that the Lagrangian of the standard model would be scale invariant, were it not for the mass term in the Higgs potential. They then construct a minimal extension of the standard model where scale invariance is spontaneously broken (or "hidden", in the terminology of Coleman), by introducing a Goldstone boson - the dilaton. Its couplings are fixed by the requirement of local scale invariance (in the presence of a gravitational field). The theory is nonrenormalizable and should be regarded as a low energy effective field theory. It is observed that the couplings of the dilaton are the same as those of a conformally flat metric, except for the sign of the kinetic term. The solution of the classical EOMs with constant, finite dilaton and Higgs field require that the potential be adjusted to be zero at the minimum. The potential for the Higgs/dilaton system has a flat direction corresponding to the masslessness of the dilaton. It is shown that quantum corrections lift this degeneracy: the full effective potential contains a Coleman-Weinberg potential for the Higgs plus a term proportional to the dilaton and the anomaly. In contrast to the classical theory, the dilaton is now massive and the potential is not zero at the minimum.

Hung Cheng,
Possible existence of Weyl's vector meson
Phys. Rev. Lett. 61, 2182 (1988)
This wonderful little paper introduces a new twist in the previous story. It starts by noting the following two reasons that would make the existence of Weyl's vector meson (no longer identified with the electromagnetic field) desirable: (1) just as the W and Z absorb the angular degrees of freedom of the Higgs doublet, Weyl's vector meson could absorb the radial degree of freedom. Then, all degrees of freedom of the Higgs doublet could be eliminated by gauge transformations (SU(2)xU(1) for the angular degrees of freedom and scale transformations for the radial degree of freedom), and the Higgs particle would not be seen; (2) it would be desirable to eliminate Newton's constant in favor of a dimensionless coupling and the VEV of the Higgs field (this is the same motivation as in Zee's paper).
The paper sketches an extension of the standard model, coupled to gravity, which uses Weyl's non-metric connection and achieves these two goals. Interestingly, Weyl's vector meson couples to gravity but not to fermions or to the other gauge fields. The paper closes with the following remark: if one chooses the Weyl gauge where the VEV of the Higgs doublet is constant, the remaining scalar degrees of freedom describe a nonlinear sigma model, which is nonrenormalizable even in the absence of gravity. Thus this theory is in a sense worse behaved that the standard model.

Very similar considerations have been developed in greater detail in

M. Pawlowski and R. Raczka,
A unified conformal model for fundamental interactions without dynamical Higgs field
Found. Phys. 24, 1305-1327 (1994)

More recently, the role of conformal symmetry in the standard model has been revisited in the following papers.

K.A. Meissner and H. Nicolai,
Conformal symmetry and the standard model
Phys. Lett. B648, 312-317 (2007)
arXiv:hep-th/0612165
Effective action, conformal anomaly and the issue of quadratic divergences,
Phys. Lett. B660, 260-266 (2008)
arXiv:hep-th/07102840

The motivation for these papers is the idea that the standard model could arise from some exactly conformally invariant theory. Then, the smallness of all known particle masses compared to the Planck scale may be due to the quantum mechanical breaking of conformal symmetry. In this scenario it is postulated that there is a "great desert" between the TeV and the Planck scale, and that all couplings are free from Landau poles in this energy range. It is shown that there are parameter choices which are consistent with this hypothesis and with known phenomenology. The Higgs mass is predicted to be above 200GeV. The second paper contains a calculation of the part of the nonlocal effective action which is responsible for the anomaly.

L.D. Faddeev,
An alternative interpretation of the Weinberg-Salam model
Talk given at "New trends in high energy physics", Yalta 2008
arXiv:0811.3311
The starting point of this paper is the action of the bosonic part of the standard model, without the Higgs potential. "The interpretation.. is exactly based on this omission". The Higgs doublet is reparametrized in terms of a singlet scalar ρ (the radial mode) and an SU(2)-valued field g (the angular, or Goldstone, modes). The field g is used together with the gauge fields to form gauge invariant vector boson fields. In terms of these variables the action contains kinetic and mass terms, plus a kinetic term for the radial Higgs mode. The functional integration over g (volume of the gauge group) is completely separated, without gauge fixing. It is observed that the radial mode enters in the Lagrangian exactly like the conformal factor of the metric. This interpretation is presented as a possible reason for the nonzero expectation value of the radial mode.

M. Shaposhnikov and D. Zenhäusern,
Quantum scale invariance, cosmological constant and hierarchy problem
Phys. Lett. B671, 162-166 (2009)
arXiv:0809.3406 [hep-th]
Scale invariance, unimodular gravity and dark energy,
Phys. Lett. B671, 187-192 (2009)
arXiv:0809.3395 [hep-th]

These two papers, together with the one by Shaposhnikov and Tkachev mentioned earlier, are motivated by the observation that in a globally scale invariant (SI) quantum field theory, large mass ratios (such as in the hierachy problem or cosmological constant problem)  would be stable under radiative corrections (there would still be a question of why these numbers are so small or large, but there would be no need of special mechanisms such as SUSY, technicolor or little Higgs to stabilize such ratios). In addition, if gravity is SI and unimodular, the cosmological constant appears as an initial condition.

One can construct a simple theory of a scalar field (the "Higgs") coupled to a dilaton and a metric, such that SI is spontaneously broken and all masses in Nature (Higgs mass, Planck mass) derive from the VEV of the dilaton, which itself would be exactly massless.
An analysis of SI unimodular gravity in Einstein frame, shows that there exist runaway solutions that can be interpreted as inflation, so the model also gives a natural candidate for dark energy. Unfortunately this scenario seems to be endangered by the conformal anomaly. In these papers it is shown that one can construct effective field theories such that (i) SI is preserved at all orders of perturbation theory (ii) SI is broken spontaneously, leading to a massless dilaton (iii) the effective running of couplings is reproduced at low energies. The trick to achieve this is to compute radiative corrections with a modified dimensional regularization scheme, along the lines of Englert et al.


G. 't Hooft,
Quantum gravity without space-time singularities or horizons,
arXiv:0909.3426 [hep-th]
Probing the small distance structure of canonical quantum gravity using the conformal group,
arXiv:1009.0669 [hep-th]

The conformal constraint in canonical quantum gravity,
arXiv:1011.0061 [hep-th]
A class of elementary particle models without any adjustable real parameters,
arXiv:1104.4543 [hep-th]

In this series of recent papers, 't Hooft puts forward some new ideas on the possible role of the conformal factor of the metric. He says in the first paper: "Something has to give, and...we claim to have found a good candidate for that: the definition of scales in space-time. It should be done in a way that differs from conventional wisdom". He considers the notion of "black hole complementarity", namely the relation between the view of an infalling observer and one sitting at infinity outside a black hole. He considers a very simple case of a black hole that forms from the collapse of a spherical shell of matter, and subsequently evaporates in another outgoing shell. By demanding that the views of the two observers be related by a local and causality-preserving mapping, he arrives at the conclusion that such a relation must consist of a conformal transformation. Thus "[the conformal factor] is observer dependent". The transformation is discussed in some detail for the simplified black hole model.

In the other papers it is suggested that the path integral should be split into two steps. The first step is the integral over the conformal factor; this should yield a conformally invariant theory of matter and gravity, which might therefore be expected to be renormalizable or even finite. The second step is the integral over matter and finally over conformal equivalence classes. The main technical issue is that the first integration is actually divergent in a way that is not easily cured by the standard techniques. After listing various possibilities, he considers of a classically conformal theory of spin 1, 1/2 and 1 fields in a flat background metric. In order to have masses without violating Weyl invariance a dilaton is also present. It is then required that the beta functions of this theory vanish. This leads to constraints on the matter couplings which in principle could fix all parameters of the theory.




Last update 29 May 2011