>Concerning your classical boundaries in a ''partially quantum universe'', I do not see any logical reasoning behind it apart
>from the desire to have classical boundary structures in order to define observables. For example, how large are these chunks,
>what physical principle decides upon that ? Moreover, for ordinary particle theory in curved spacetime, no such boundaries are
>present (and would destroy the coherence of the theory) except at asymptotic infinity which is held flat or de Sitter.
I have never mentioned classical boundaries, nor partially quantum universes, whatever that means. I wrote that the formalism allows to consider finite open regions of 'spacetime', with their boundary (quantum) geometry and topology fixed, and bulk geometry and topology fluctuating and dynamical. Indeed, a better understanding of classical and quantum field theories in such generalized context is needed, together with the corresponding possible generalization of standard quantum mechanics. Such generalization, however difficult, seems interesting, if not necessary, to me also beyond this specific approach.
>Third, the inclusion of matter needs to break general covariance in one of the following senses:
>(a) either you have a diffeomorphism invariant dynamics (that is a new constraint algebra containing the matter variables) but
>you have to resort to partial observables.
> (b) the quantization of gravity with matter will induce anomalies in the algebra.
>Concerning the constraint algebra, this question has not even been settled in pure gravity theory because the quantization
>procedure treats the Hamiltonian different from the spacelike diffeomorphism constraints. Concerning (a), this is physically
>nonsensical because I do not see how you would retrieve an arrow of time in this way.
none of the above is correct, in my understanding. The use of partial observables is a more convenient way to deal with Dirac observables, and to understand their meaning as correlations of measured (but not diffeo invariant) quantities. It does not imply any lowering of standards with respect to covariance. One can produce explicit quantizations of the constraint algebra of gravity plus matter which are free of anomalies, and the real question is whether the corresponding quantization has the correct classical limit and produces the correct physics. But there is no obstacle of principle.
>Fourth, I did not say that pure gravity was ill defined, I simply said it has no observables; it is an empty theory from the
>physical point of view, while the limit of zero gravity is not and that is actually the correct vacuum.
I did not question the fact that pure (classical and quantum) gravity is non-physical, because we lack local observables, although I would not be so clear-cut; and in fact I said that this gives one more reason, beside the obvious physical motivation, to introduce matter. I wrote that just as in classical GR pure gravity does represent an idealized case from which we learn things, the same could be true in the quantum case. The limit of zero gravity is physical provided you are not interested in gravity (classical or quantum), which is a shame. As soon as you want to say something about gravity, this limit becomes at best an approximation, as one does in any interacting field theory, and all the problems re-appear and have to be dealt with.
>Fifth, I do not know of any standard approach to quantum theory which is not grounded in a classical theory. The path integral
>approach has the classical action as starting point and likewise so for the Hamiltonian one. The only kind of reasoning which
>departs from quantum concepts partially (but not fully) can be found in the book of Weinberg.
sure. and in fact -any- approach to quantum gravity I know of (including GFT) rests to some extent, in motivation, type of structures used, basic principles that one tries to carry over to the quantum theory, etc on classical GR. again, I never stated that one should somehow invent a quantum theory of gravity and/or spacetime without ever considering GR. so what?
>Asymptotic freedom is just the physical idea that on short distance scales the theory becomes a free one. This is a well defined
>concept in a quantum as well as classical setting.
in my understanding the concept makes real sense only in a quantum theory in which coupling constants run with scales, otherwise you are using the term in a rather non-standard way. Then, QCD is asymptotically free while QED is not, and none of the two is 'asymptotically free' at the classical level, given that there the coupling constants are whatever one sets them to be. In any case, Gravity, treated as a standard quantum field theory, is not asymptotically free, although it could be asymptotically safe. This is true, of course, unless you treat it as a non-standard quantum field theory or you intend the terminology in a non-standrad way. Fine, but you should then clarify what you mean, and then one can check whether what you mean makes sense or not.
>Finally, relativity was found by reasoning in terms of a new principle. Einstein clearly thought about general covariance and
>there exist plenty of historical documents to prove that. I am not sure about the person, but I remember he told to Planck about
>a generally covariant law for gravitation and the response was that nobody would be interested in that.
>Moreover, you completely miss the point that finding principles is very difficult because it implies that your really know what
>you are doing physically.
when I read the historical texts or the original sequence of articles leading to GR, I see a much more complicated story, in which he arrived at the right principles only after a complicated sequence of trial and errors, partial results, later-to-be-discovered inconsistent foundations, glimpses of ideas, and even including formulations of the theory that were based on the very contradiction of the principle of general covariance. He did not first identify the principles and then deduced the results. Theoretical physics does not work like that, I think, unless principles are treated as working hypothesis, but then of course one should maintain a certain flexibility about them. This is exactly because identifying the right principles is difficult (again, I have never stated the contrary), and it is not even something that can be recognized as unique, if not much after the complete theory has been found. As a consequence, I do not feel I can blame any current approach to quantum gravity (a still incomplete theory, yet to be found, really) because it does not start from unique principles, or on already clear ones. Obviously, I also feel it is important to try to clarify the basic assumptions (''principles'') on which they are based, because indeed it may facilitate their development.