Yes, but there’s still some terminological sleight-of-hand going on here. It is only fair to say that a future A affected a past B if P(B) is well defined without reference to A. In this case it’s not. Because B is defined in terms of correlations between measurements made at T1 (noon) and measurements made at T2 (evening) then B cannot be said to have actually happened until T2.
correlation is a two-way street
No, it’s an n-squared-minus-one-way street. It appears to be a two-way street in one (very common) special case (two macroscopic systems mutually entangled with each other), but weak measurements are interesting precisely because they do not conform to the conditions of that special case. When you go beyond the conditions of the common special case you can’t keep using the rhetoric and intuitions that apply only to the special case and hope to come up with the right answer.
Yeah, probably. It’s actually probably N!-1 because you have to trace over one degree of freedom to obtain a classical universe. But the details don’t really matter. What matters is that it’s >>N.
Yes, but there’s still some terminological sleight-of-hand going on here. It is only fair to say that a future A affected a past B if P(B) is well defined without reference to A. In this case it’s not. Because B is defined in terms of correlations between measurements made at T1 (noon) and measurements made at T2 (evening) then B cannot be said to have actually happened until T2.
No, it’s an n-squared-minus-one-way street. It appears to be a two-way street in one (very common) special case (two macroscopic systems mutually entangled with each other), but weak measurements are interesting precisely because they do not conform to the conditions of that special case. When you go beyond the conditions of the common special case you can’t keep using the rhetoric and intuitions that apply only to the special case and hope to come up with the right answer.
You’re right. Good point.
Don’t you mean n-factorial? Anyway, … hmm, I need to think about this more.
Yeah, probably. It’s actually probably N!-1 because you have to trace over one degree of freedom to obtain a classical universe. But the details don’t really matter. What matters is that it’s >>N.