colorSpace said:
jVincent said:
What one needs is to construct experiments, that exhibit behavior that is impossible under a hidden-variable model.
Your wish has been heard, see my above messages.
In the terms of the debate that are set by the words "hidden-variable model", I agree with colorSpace, up to
extremely slight concerns about the detection loophole and up to an acknowledgment that de Broglie-Bohm and Nelson trajectory models are more-or-less viable, but unattractive.
If the terms of the debate are that we are interested in classical models for the observables of an experiment that violates experiments, not so much. For example, the Copenhagen interpretation insists that there must be a classical record of an experiment, that a quantum theoretical description must be in correspondence with that classical record. That is, there are classical
non-hidden-variable models for experiments, and according to the Copenhagen interpretation (without too much commitment to the Rolls-Royce of interpretations) there
must be.
The question put this way can be extended by asking whether there are other variables that are currently not measured, but could be. Clearly there always are: we could measure the position of the leaky oil can that's sitting on top of the experiment casing, and determine whether moving the oil can changes the results of the experiment (probably we would rather just move the oil can out of the room, don't people know that opening the door changes the results? Who left this oil can on top of my experiment anyway?) So that's an unmentioned classical observable (non-hidden-variable) that could be measured, we just didn't yet.
Now comes the million dollar question, just how many observables are there in a classical model? A classical Physicist, informed by 20th century Physics, would presumably answer that there is potentially unlimited detail, that one choice would be to describe the experiment using a classical field theory. Unfortunately for the classical Physicist, we don't have classically ideal measurement apparatus that can measure arbitrarily small details without changing other results, if we bring in the STM to measure the positions of atoms in the walls of the vacuum chamber that contains the experiment, we pretty much have to dismantle the apparatus to do it; when we put it back together, after we've measured the precise position of every atom, someone will contaminate the surface with the leaky oil can, so we might as well not have brought in the STM at all.
Why doesn't a classical Physicist have a classically ideal experimental apparatus? The answer, it seems, is that we can reduce the temperature (the thermal fluctuations) of an apparatus as much as we like, but we cannot reduce the quantum fluctuations of the apparatus at all, so we can't reduce the interactions of our classical apparatus to as little as we like. In classical modeling, if we cannot for some reason reduce the temperature of the measurement apparatus, and the thermal fluctuations of the measurement apparatus do affect the results of the experiment, we model the thermal interactions of the measurement apparatus with the measured system explicitly.
In experimental terms, although we can reduce the temperature of an experimental apparatus as much as we like, we cannot in fact reduce the temperature to absolute zero -- no thermal fluctuations at all. Nonetheless, we act as if we can, because we can determine the thermal
response of the Physics,
the way in which the results change as we reduce the temperature. Extending that response to the absolute zero point is problematic, since we have no idea whether the Physics changes drastically as we get closer to absolute zero (the response of He to temperature changes at 10K tells us almost nothing about the response at 1 mK, for example), but we do it anyway. Extending the thermal response to absolute zero from our current best measurements is an idealization that we work happily enough with.
I now want to link this thread to another, [thread]205586[/thread], where I ask "Are there cosmological models in which Planck's constant varies?" A response to that thread clarified my ideas considerably, and has significance here. The general idea is that a change of the metric in a model can be understood to be equivalent to a change of the level of quantum fluctuations. In particular, when we claim that the metric changes as we move in a gravitational field, we invoke a particular coordinatization; in a different coordinatization, we would say that the amplitude of quantum fluctuations changes as we move in a gravitational field, while the metric remains constant. Quantum fluctuations affects everything, just as metric variation affects everything. In the context of this discussion of measurement and Bell inequalities, this means that although we cannot reduce Planck's constant as much as we like, we can determine the quantum fluctuations
response, given a coordinatization in which we consider a metric field to be constant while thermal fluctuations change when we move an experiment in a gravitational field.
I had no idea my argument would go this way when I started this post. If we can determine the quanthal response (I've just coined this word as a quantum equivalent of the word thermal, but it doesn't seem special) of an experiment by moving an apparatus around in a gravitational field, it becomes reasonable to talk about what we would observe if we had an ideal classical apparatus at zero quantum fluctuations.
That's a little wild.