Haelfix said:
Glanced through the paper. He wants to relax positive semi definitiveness of the Hamiltonian, and not demanding the Poincare group to act continously on the derived Hilbert space. Also, these random Lie fields are essentially classical objects. Of course when you make your life difficult like that, reproducing even standard things (like Fermions) becomes highly tentative. Also there's nothing really to discuss yet, he makes no claim about whether or not this can model anything we know off.
Anyway that's fine, its interesting to see where the math takes you and see if its useful for modeling something physical, but the task of reproducing 40 years of nontrivial and observed quantum effects that have no apparent classical analogs still remains as an 800 lb gorilla in the room (like say anomalies). Heck, constructive field theorists after decades of trying with far stronger and more natural constraints can't even prove the existence of a single physical field theory in 4d, much less tackle any sort of phenomenology. Its just one of those fiendishly difficult topics in physics.
Thanks Haelfix, and thanks Marcus for the OP.
Although I'm careful to mention the lack of a continuous action of the Poincare group on the Hilbert space, I personally think this requirement is a mathematics too far in conventional axiomatizations, and is not a substantial limitation of the mathematics. I believe the restriction to a finite number of test functions could be taken away without special problems. I had an exchange with Fredenhagen, Rehren, and Seiler a year or two ago in which I queried the lack of a requirement for a continuous action in their paper http://arxiv.org/abs/hep-th/0603155" . They require only "covariance under spacetime symmetries (in particular, Lorentz invariance of the dynamics)", but of course in correspondence it turned out that to them
of course this means a continuous action. Still, I think calculations in perturbation theory, and practical calculations generally, never use the availability of a continuous action.
I'd take small issue with the idea that "far stronger" constraints are "more natural". The restriction to positive frequency is just that, a restriction of the class of models we are willing to consider. If we take away this restriction, it gives us other models to consider. I'm just now pulling apart Hans Halvorson's and David Baker's paper http://philsci-archive.pitt.edu/archive/00004467/" , which gives as clear an analysis of complex scalar free QFTs as I've ever seen. In order to make a complex scalar free QFT have positive energy, they have to introduce a complex structure that could
only be natural if you're
determined to make the energy positive. If the vacuum is stable for thermodynamic reasons, not because there are no lower energy states for it to decay into, one can use the natural complex structure. The vacuum state gives probability densities for observables and for joint measurements of compatible observables because the inner product is positive semi-definite (I keep a Hilbert space structure, after all), but the Hamiltonian does not have to be positive semi-definite for there to be a sensible probabilistic interpretation of the mathematics.
I note that the Hamiltonian is irrelevant to calculating the Wightman functions in the vacuum state of a free quantum field. We only need the commutation relations between creation and annihilation operators to calculate everything. Of course, creation and annihilation operators are not observables, they are theoretical objects that are used pervasively in perturbative QFT, quantum optics, and almost all practical applications of QFT, but they are definitely not used in algebraic QFT. Also, the deformation that I'm discussing is definitely a baby step, insofar as other deformations of the creation and annihilation are possible. Of course, eliminating the Hamiltonian from all our discussions changes things a little, but I think it's all good to have a mathematics that is so different, because it puts what we have been using in such sharp perspective.
Haelfix: I would be interested to know what you think we might weaken in the Wightman axioms (or in the Haag-Ruelle axioms, if you prefer)? [I think it's not unreasonable to answer that people should continue to try to construct a rigorous concrete QFT that satisfies the Wightman or Haag-Ruelle axioms, but I would like whatever is produced to be comprehensible and tractable after the fact.]
As far as Fermions are concerned, I think I will have to say that they're only observable by their effects on bosons and the consequent effects of the bosons on thermodynamically metastable mesoscopic or macroscopic collections of fermions and bosons (which are called detectors), since we cannot construct gauge invariant observables out of Fermion fields alone. If the phenomenology that we have become accustomed to attributing to Fermions can be modeled in a different way, I'd like to see it. It would of course, if it's possible, lead to a change in our understanding about as great as removing our reliance on Hamiltonians. [I know this is evasive, but I've only been working ten years on my own so far. String theory has had tens of thousands of physicist-years of ingenuity and hard work. Of course if tens of thousands of Physicist-years are expended on the mathematics of random fields, we may have as much to show for it as we would have if we expended the same effort on the worst kind of crank theory. The sociology of the adoption of an idea fascinates me as much as it fascinates any crank, almost as much as whether the mathematics is consistent.]