Calculating observables in a quantum field theory is a subtle process that must be done correctly and "correctly" means to be careful about the right physical interpretation and required physical properties of the theory at each moment (or at least the final moment when we release the results).
You are implicitly talking about theories that are constructed out of their classical limit. The right guide to construct the quantum theory and its observables is to do everything to obey the actual physical criteria, not to do some mindless operations of "quantization". When we do things correctly, we are really solving the puzzle "what is the right full quantum theory that has a certain classical limit" and we must realize that there is no fully universal and mechanical "recipe" to find the answer. One has to preserve the unitarity and gauge symmetries (decoupling of unphysical polarizations of particles), Lorentz symmetry, and other things we expect to hold in the quantum theory. This dictates how everything is treated; it also implies that we must do regularization, renormalization, and we may discover some new parameters that enter into counterterms etc.
When it's done correctly, every classical starting theory produces the same quantum theory or the same set of quantum theories (or it can be proved to be incompatible with quantization, e.g. in the presence of gauge anomalies). A particular formalism is just a tool, not the master.
In particular, when you talk about auxiliary fields, they are unphysical degrees of freedom in the quantum theory for pretty much the same reasons as they are unphysical in the classical theory. First, it is not really true that quantum mechanically, the fields don't obey the equations of motion. They do. In the Heisenberg picture, the operators obey the Heisenberg equations of motion. They're formally the same equations as those in classical physics, with hats added (operator equations). In particular, auxiliary fields obey non-differential i.e. non-dynamical, algebraic equations and they're unphysical. They don't produce new degrees of freedom. (One must first construct the Hilbert space and auxiliary degrees of freedom, having no canonical momenta because of the absence of derivatives, never make the Hilbert space any bigger.)
In the Feynman path integral approach, the path integral over auxiliary fields is an infinite-dimensional ordinary integral that treats each spacetime point separately from others. So it may be simply integrated over them whenever you calculate the amplitudes, whether they're scattering amplitudes or Green's functions or something else. What is special about the auxiliary fields is that they don't have derivative terms in the action; they don't propagate. For that reason, they don't produce any propagators in the Feynman diagrams, either. Equivalently, you may say that the propagators for the auxiliary fields are "infinitely short" in all the Feynman diagrams so they get attached to the vertices. The attachment of these short propagators to vertices is a visual way to express the fact that you're solving them; you are just expressing the auxiliary fields that enter vertices as functions of the other fields. (These "shrunk propagators" appear e.g. if you describe a supersymmetric theory by the Feynman rules in the superspace and reinterpret the Feynman diagrams in the language of Feynman diagrams for component fields.)
You may imagine that the auxiliary fields are very massive fields. Why? Because the coefficients of their mass terms (terms without derivatives but I mean not only the bilinear ones here) are much larger than the coefficients of their kinetic terms (with derivatives) and the ratio is nothing else than the masses (or squared masses for bosons). This analogy tells you that the auxiliary fields, much like the very massive fields, are first "integrated out" of the Feynman path integral.
Quite generally, there is some freedom and "lack of complete rigor" in the semi-mechanical procedures used in quantum field theory. But the general idea, as I said, is to guarantee that we produce a consistent quantum theory with the given classical limit and the required symmetries. For this reason, classically equivalent starting points are meant to produce the same final quantum product, too. Auxiliary fields and various fields redefinitions are examples of the "classical reformulations" that can make the quantization harder or easier. Both examples exist.
You may surely think of artificial examples in which it's simply possible to get rid of the auxiliary fields and obtain a theory whose quantum calculations are easier and spoiled by fewer subtleties. In that case, you should do it. You may also avoid it and get the same quantum results at the end but you will have to deal with unnecessary extra subtleties along the way. However, there are also the opposite examples. Auxiliary fields may simplify one's life.
The Nambu-Goto action, a starting point of string theory, is a great example. This action is proportional to the area of the two-dimensional world sheet spanned by the propagating one-dimensional string in the spacetime (it's multiplied by a constant known as the string tension). The proper area is an integral of a square root of the determinant of the induced metric (from the spacetime to the world sheet) and it is a horribly non-polynomial action that would be hard to quantize. However, one may describe the system in an equivalent way, using an extra degree of freedom, an auxiliary metric tensor on the world sheet (whose equations of motion simply say that it's equal to the induced metric from the $X$ fields, up to an overall scaling of the tensor), and the action actually acquires a transparent quadratic (bilinear) form.
In the right variables, it is a free theory! This bilinear action with the usual Klein-Gordon-like kinetic terms for the scalar fields $X$ describing the embedding of the world sheet in the spacetime (Polyakov action if we also include the Faddeev-Popov ghosts) is easy to be quantized. The final product, perturbative string theory, may be viewed as the quantization of the non-polynomial, square-root-spoiled Nambu-Goto action, too, although we didn't apply a mechanical quantization procedure to the Nambu-Goto action directly and mindlessly.
Auxiliary fields often simplify the calculations and reduce the technical subtleties. After all, one component (and, in some counting, two components) of any gauge field potential may be viewed as an auxiliary field; the number of physical polarizations of the photon is just two, fewer than the 4 components of the potential $A_\mu$. However, using the whole $A_\mu$ including some unphysical components – which become ordinary auxiliary fields if we add some gauge-fixing terms – is a way to preserve the manifest Lorentz symmetry of the Maxwell system and its excitations, photons.
This post imported from StackExchange Physics at 2014-05-01 12:21 (UCT), posted by SE-user Luboš Motl
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