vanesch
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colorSpace said:From my point of view, the impression is that you try to sell the idea that the concept of local splits in MWI gives you a way to explain entanglement in a local fashion for free.
I don't buy especially the "for free" part, and so I don't buy the whole package.
The property of locality is a mathematical property of a theory. It essentially means that you can find a map f from E^3 into a set of mathematical structures (ANY structures) in such a way that the temporal evolution of, say: f(p) (p is a point in E^3) and f(p) is a mathematical structure is only a function of all the f(q) with q in a neighbourhood of p in E^3, and also such that physical observations and so on done at point p in E^3 are only a function of the mathematical structures f(q).
If you can show that such a map f exists, and that it gives rise to a dynamics which is equivalent to the dynamics of your theory, then your theory has the property of locality.
It is this mapping which I established, by showing that we could associate mathematical structures (kets + a label system) to points in space (or neighbourhoods of points in space) in such a way that this is equivalent to the dynamics of the quantum formalism of non-relativistic QM in the Schroedinger representation, as long as the hamiltonian (or its integration, which is the unitary time evolution operator) is build up using only local interactions.
So once this has been shown (as in "mathematical proof") you can go back to standard quantum formalism with its global hilbert space, you KNOW that it has the property of locality - in the same way as you can continue doing Hamiltonian dynamics in 6N dim phase space, knowing that it has a local representation in E^3, even if that seems more clumsy to work with.
In addressing the measurement-problem in the Copenhagen interpretation, and its randomness, AFAIK, MWI has criticized CI for not having gears and wheels in the 'collapse' concept. So MWI should take such questions seriously.
The problem in CI is that no rule exists to prescribe when a physical interaction is to be treated one way ("measurement") or the other ("dynamics"). I don't have such a problem in what I presented: the rules are very simple, and universal.
But what is more, when considering a collapse, such as in CI, THEN you cannot find such a "local" map f(p) anymore. It is impossible to find a local representation, no matter how clumsy, in which a genuine collapse occurs. As such, the projection, in CI, is strictly non-local.
Now, why do we cling so much to locality ? What could one care ? In a purely Newtonian setting, not much. Newtonian mechanics is non-local. Forces act between "things at a distance". There exists a nice, consistent extention of Newtonian mechanics which includes quantum effects: it is Bohmian mechanics. It is explicitly non-local.
The problem we have with non-local theories is when we want to go relativistic. Because in relativity, all mathematical objects representing physical things have to live on the spacetime manifold - it is the basic idea of relativity. As such, no "non-local" objects are allowed. If you introduce them in relativity, you run in all kinds of paradoxes, such as being able to kill your grandpa and so on. This is why "locality" is such an important thing. You can hope to extend a local theory into relativity. You know that a non-local theory will bring you troubles.
Now, you can say, if we find experimentally that nature is non-local, then so be it. Right. But we've seen that the ONLY aspect of non-locality in quantum theory comes about by the interpretation we give to it. From the moment that there is a projection, there is non-locality (no hope to implement a relativistic version). But if we don't do projections, and we keep with the unitary dynamics, then we have seen that locality is preserved. So it is premature to say that quantum mechanics is non-local, as the non-locality is imposed only by an aspect which is discutable: projection.
Given that in MWI, you DON'T use projection, you can still keep the locality property, and as such, the extension to a relativistic theory.