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If anything, my position is more extreme than Rovelli's. The problem with quantum gravity is that QM, or rather QFT, is not completely quantum - there is an residual classical element which causes problems. **
Not in the path integral formulation (see later).
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This is most easily seen in the Hamiltonian formulation. Here one starts by foliating spacetime into fixed-time slices. But since time is defined by the observer's clock, this step implicitly assumes the existence of a macroscopic, classical observer. **
I do not see why (the foliation is a problem for quantum covariance in the Hamiltonian formulation true), doing QFT on any background *should* (at least according to our wishes) not be dependent upon the choice of foliation (that is the theories are expected to be unitarily equivalent) - this is not true in case of the thermal state calculated in the context of the Unruh effect of course, but the latter is due to a singular coordinate transformation.
** One can of course pick another foliation, which corresponds to a different choice of observer, but once time has been defined, it remains the same independently of what happens. **
Ok, but physical measurements should be independent of choice of global foliation in background dependent QFT (they indeed depend only upon the local classical clock of the observer).
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This is an unphysical assumption. In order to observe a system, the observer must interact with it. This interaction will transfer momentum to the observer, making her undergo a Lorentz transformation, and change the definition of time. Thus, the act of observation changes the foliation. Only if the observer is macroscopic, and thus classical, can we ignore this effect. **
You mean the LOCAL foliation I presume.
Ok, but in an entirely classical theory, it would be ``easy´´ to calculate such backreaction effects and even in the context of QFT one could calculate the higher momenta of the momentum transfer and impose - as a first order correction - accordingly a statistical motion upon the observer (this not a local procedure in the strict sense of course but the same would be in the quantum case). More general: within the framework of Hartle and Sorkin, you basically only need an initial hypersurface and wave function to ask any spacetime question concerning any field observable you want to (on a fixed spacetime background) given a certain notion of coarse graining. This does not depend upon any foliation at all, you can treat everything quantum.
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This is not so serious if we ignore gravity, since detectors are usually much bigger than the quantum phenomena we want to observe. However, a macroscopic observer has infinite mass. Hence the assumption about an a priori foliation secretely introduces an infinitely massive observer into the universe. **
No, it does not, the foliation is entirely kinematical.
**Since gravity interacts with this infinite mass, this assumption will most likely wreck havoc in a quantum theory of gravity, in agreement with experience.**
No, something like CDT has a classical time notion and some observables come out right.
** One may expect to recover ordinary QFT from observer-dependent QFT in the limit that the observer's mass goes to infinity, in the same sense that one recovers Newtonian mechanics from QM when hbar -> zero and from SR when c -> infinity. **
Classical mechanics cannot be retrieved from quantum mechanics (for N particle systems), taking limits can a be subtle and nasty process.
Cheers,
Careful