secur said:
... the essential peculiarity of QM, compared to classical, is that in order to completely predict results, info beyond the past light cone is required.
A. Neumaier said:
One needs the information on a Cauchy surface, not on the past light cone, to make predictions. More precisely, to predict classically what happens at a point in the future of a given observer, the latter's present defines (at least in sufficiently nice spacetimes) a Cauchy surface where all information must be available to infer the desired information.
First let's get Closed Timelike Curves out of the way. It occurs to me that their presence might vitiate my statement, depending how you look at it. They're not supported by experiment and thoroughly irrelevant to this discussion. So let's ignore such pathological spacetimes.
Then we can, as you say, define a Cauchy Surface for any observer, for instance Alice or Bob in typical Bell experiments. But this contributes nothing to the discussion.
Cauchy Surface is used to formulate an "Initial" Value Problem in GR or SR, to determine a complete solution (both past and future) for an entire space. The spacetime point or event where/when Alice makes her observation is one point on a Cauchy Surface which constitutes her "instant" (loosely speaking) throughout space. The info at that specific point comes only from her past light cone (assuming "forward" time). To predict her result, all the rest of the Cauchy Surface is irrelevant (classically) since by definition it can't causally affect her. If we're interested in solving Einstein Field Equation for the entire block universe we'd need it - but we're not.
So (ignoring Closed Timelike Curves) you're simply wrong. One does NOT need the entire Cauchy Surface (which includes detailed info on the Bullet Cluster, for instance, which won't affect her for 3.7 billion years) to predict what Alice's SG says about her particle today in a lab here on Earth!
A. Neumaier said:
it is no different in quantum mechanics when one makes (probabilistic) predictions.
Sorry, that's irrelevant, since my statement is about
exact (implied by the word "completely"), not probabilistic, predictions.
A. Neumaier said:
The apex of the light cone is the point in space-time at which all information needed to do the statistics is available.
Correct. That apex is precisely Alice's measurement's spacetime event. All the info there is determined by her past light cone, and nothing else - classically.
To summarize - arguably, with GR, you can produce a contradiction to my statement. In a pathological spacetime one could argue that classical predictions at a point require info outside the past light cone - maybe. If so, I'll concede the point. The fact one must go to such extremes demonstrates the basic validity of my statement.
Cauchy Surfaces have nothing to do with the discussion of my statement (which, I claim, is quite illuminating), or of Bell-type experiments (excepting GR-related Orch-OR and Joy Christian :-), or of Gell-Mann's video. Let's not muddy the waters with irrelevancies, it's muddy enough already.