A. Neumaier said:
I misstated in #16 what I had meant to say; see the updated formulation there for the intended version. To derive Bell's inequality you need to make assumptions that are never satisfied when you start with Maxwell's equations. Thus Bell's inequality doesn't hold. But the quantum result is just based on properties of the Maxwell equation, hence the quantum field approach gives identical results with the experimental findings.
I'm not sure what you're saying here. It seems to me that the assumptions behind Bell's inequality can be formulated in a way that is independent of the distinctions between particles and fields.
Roughly speaking, let's assume SR (GR causes complications that seem irrelevant). Pick a rest frame. Pick a time interval \delta t. Now, relative to that rest frame, partition space into cubes of size c \delta t.
Let \mathcal{R} be the set of all possible records, or histories, of a single cube during a single time interval. So classically, a record might consist of an identification of what particles were in the cube during that interval, what their positions and momenta were at times during the interval, what the values of various fields at different points within the cube were at times within that interval.
From classical probability and special relativity, we would expect that if \mathcal{R} was a complete description of local conditions within a cube during an interval, then the behavior of the universe can be described by a grand transition function \mathcal{T} : \mathcal{R}^{27} \times \mathcal{R} \rightarrow [0,1]. The meaning of this is that \mathcal{T}(\vec{r}, r') is the probability that a cube will have record r' for the next interval, given that it and its neighboring cubes have record \vec{r} during the current interval. So this is just saying that the behavior of a cube during the next interval is dependent on the behavior of its neighboring cubes during this interval. Note, I'm allowing the behavior to be nondeterministic, but I'm requiring the probabilities to be dependent only on local conditions. Also, I'm being sloppy about talking about probabilities, since in general there could be (and would be) uncountably many possible records. So I should be talking about probability distributions, instead of probabilities.
The two assumptions that (1) \mathcal{R} is a complete description of the conditions within a cube during an interval, and (2) Einstein causality, imply that knowledge of conditions in distant cubes can give you no more information about future possibilities for one cube than knowing about conditions within neighboring cubes. Putting that more coherently: I pick a particular cube. If I know about conditions in that cube and all its neighboring cubes during one interval, then I can make a probabilistic prediction about conditions in that cube during the next interval. Those probabilistic predictions cannot be changed by more knowledge of conditions in non-neighboring cubes. This basically makes the universe into a gigantic 3D cellular automaton (except for the fact that the records are pulled from an uncountably infinite set, while the theory of cellular automata require the records to be taken from a finite set; I'm not sure how important that distinction is for the purposes of this discussion).
Completeness is an important assumption here. Obviously, if my records are incomplete---that is, there are microscopic details that I failed to take into account--then it is possible that additional correlations between distant cubes could be implemented by those microscopic details, which would give the erroneous appearance of nonlocality. If I took those microscopic details into account, then local information would be sufficient to predict the future of a cube.
Bell's theorem applied to the EPR experiment shows that it can't be described this way, and that it can't be fixed by assuming microscopic details that we failed to take into account. In the EPR experiment, no matter how fine-grained your descriptions of the cubes, information about conditions in distant cubes can tell you something about the future behavior of this cube.
But getting back to your point about Maxwell's equations, it seems to me that there is nothing about my "cellular automaton" model of the universe that would prevent the use of the electromagnetic field as part of the record for a cube.