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fzero
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marcus said:This all makes sense, and is certainly good to know, if only as historical basis.
But what interests me is that if you look at the new formulation, which has appeared only since 2010---say you look at the pedagogical review 1101.3660 that A. Neumaier just referenced---then where is the [tex]\mathbb{R}\times \Sigma[/tex] manifold?
Where are the Ashtekar variables? Where are the holonomies? Where is the old configuration space of pre-2010 Loop Gravity?
The metric operator in (22) of 1102.3660 is 3x3. This corresponds in some way to the metric that Ashtekar decomposes into the spin connection, possibly explained in the paper
http://arxiv.org/abs/gr-qc/9411005 where Rovelli and Smolin made the connection with spin networks.
I believe that the states in [tex]\mathcal{H}_\Gamma[/tex] are the holonomies, see the remark under equation (18) where this is identified with the Hilbert space of lattice gauge theory.
This is the point I was trying to make by the way I responded to Neumaier's question. It is actually very interesting. We have this new very concise formulation, with little or no "extra baggage". It is expressed in just a few equations---with Hilbertspace and operators defined in a rather direct transparent way.
In this new formulation, the question is very relevant---how do we know the dimensionality?
A. Neumaier refers to what it says right after equation (23) on page 4 of http://arxiv.org/abs/1102.3660 . Where paper [8] by Penrose is cited.
I think this may be the right place to look.
I think whatever connection this model has with canonical gravity is still related to the old one of Rovelli and Smolin. I don't know what makes it a new formalism, so I can't say what refinements of the old ideas are there. It may not start with the Ashtekar formalism, but the same type of formulas come up if you want to relate quantities in the [tex]SU(2)[/tex] variables to the metric. There could be differences in quantum theory, but the semiclassical physics probably agrees.