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bhobba said:The tricky part of this is, while it is often said the rules of GR and QM are incompatible, the truth is they really aren't:
http://arxiv.org/abs/1209.3511
Its a modern insight from the effective field theory view of re-normalisation sorted out by Wilson.
I'm not sure that all the problems of reconciling GR and QM are due to non-renormalizability. Certainly that's part of it, and you're probably right, that that part is exaggerated, because nonrenormalizable theories just mean that our theory is incomplete--it's just the low-energy limit of some unknown theory of wider applicability.
But a couple of things about GR seem to call into question some basic fundamental aspects of QM. They are completely over my head, so I can't engage in a meaningful discussion about them, so I'll just mention them.
- The problem of "time and observables". As I said, this subject is over my head, so my summary is probably misleading or wrong, but as I understand it, the problem is that QM understands dynamics as the evolution of a quantum state as a function of time, while there is no unique, satisfactory time parameter, according to GR. Another, related problem is that QM is about expectation values and eigenvalues for observables, but for the gravitational field itself (or spacetime curvature), there is no obvious notion of "observable" that is local and coordinate-independent.
- The problem of information. I don't know enough to know whether this is connected with the first problem, or not, but it's easy enough to describe. According to QM, information is never lost, at the microscopic level, since the equations of motion are reversible. In contrast, black hole formation and evaporation through Hawking radiation seems to involve information loss: the information about what went into forming the black hole is gone forever, since regardless of what falls into a black hole, the black is only characterized by total mass, total charge and total angular momentum.