Thanks for the page reference! I see you chose a negative paragraph out of Livine's tutorial/survey of spinfoam LQG. Here is the rest of the page 54 section surrounding it, to give context and provide balance:
==quote Etera Livine
http://arxiv.org/abs/1101.5061 ==
3.1.2 The Practical Calculations of the Graviton Propagator
This framework for the spinfoam graviton propagator is based on a very simple setting. There has been a lot of research work done on this subject. Results are, up to now, both full of promise and very restricted.
On the positive side, we are able to compute systematically at leading order the spinfoam graviton propagator at large scale (for large values of the boundary areas j∂) for all the spinfoam models which have been defined. We have even developed techniques to extract (in principle) all quantum corrections of arbitrarily higher order (interpreted as “loop corrections”). This leads to recover the proper scaling of Newton’s law for gravity, with the gravitational potential going as the inverse distance, and even the correct spin-2 tensorial structure of the graviton (correlations) for specific spinfoam models. We even understand the relation between the spinfoam path integral and Regge calculus at large scale. The short scale behavior has also been investigated. It appears that the graviton propagator is regularized (as expected) by quantum gravity effects and that we have the emergence of a dynamical minimal length scale close to the Planck scale. All this has been tested analytically and numerically.
On the negative side, the actual setting for practical calculations of the spinfoam graviton correlations has been much too simple up to now. These basic calculations were done mainly for a single 4-simplex, which is indeed the simplest space-time triangulation. They typically do not involve summing over bulk internal associated to internal spinfoam vertices. Thus, these calculations don’t allow to truly test the quantum gravity dynamics defined by the spinfoam models and the gluing of 4-simplices (“space-time atoms”) used to construct the amplitudes. They should be considered as kinematical checks. It thus remains a challenge to go beyond the single 4-simplex and work with refined space-time triangulations, which would allow local fluctuations of the curvature in the bulk.
Here is nevertheless a (almost-exhaustive) list of the works done on the programme of the
spinfoam graviton propagator:
• Definition of the framework [81, 82].
• Analytical study of the asymptotic ansatz for the spinfoam vertex amplitude in order to recover at leading the correct tensorial structure for the graviton propagator [83, 84, 85].
• Group integrals techniques to compute explicitly analytically the graviton propa- gator for the Barrett-Crane model (generalizable to arbitrary spinfoam models ex- pressed in the connection representation) [88].
• Numerical investigations of the behavior of the graviton propagator for the Barrett- Crane model, both for the large scale and short scale, both at leading order and at next-to-leading order (first order quantum gravity corrections) [89, 90]
• Calculations of the asymptotics of the graviton propagator for the EPRL-FK spin- foam model [91].
• Definition of a 3d toy model using the Ponzano-Regge model [92], numerical investi- gations and development of the tools to compute the full expansion of the correlations and solve the model analytically [93, 94].
• Study of the propagation of coherent wave-packets of geometry within a 4-simplex [95].
• Analytical and numerical study of the asymptotics of the spinfoam vertex amplitude relevant to the calculations of the large scale behavior of the graviton propagator, in 3d [96, 97] and in 4d for both the Barrett-Crane model [98] and the EPRL vertex amplitude [99, 100, 101].
• Discussion of the potential use of the recursion relations satisfied by the spinfoam vertex amplitudes to the computation of the graviton correlations and to derivation of Ward-Takahashi identities for spinfoam amplitudes [97, 102].
• Tentative calculations of the 3-point correlation functions [103].
What is very nice about this framework is that it provides a physical interpretation to the correlations computed using spinfoam models and in particular shows how to recover the classical Newton’s law for gravity from our complicated and intricate model for a quantum gravity path integral. Moreover, we can actually compute analytically these correlations, plot them numerically, check that everything is consistent, and see explicit the first elements of the spinfoam dynamics with our own eyes.
However, progress in this direction is completely coupled with necessary progress that needs to be done on the coarse-graining and renormalization of spinfoam models. Indeed, we need to be able both to repeat the same graviton correlation computations for more refined and complex bulk triangulations and to say something about the non- perturbative sum over all 2-complexes. The main hope for this is put in exploiting the group field theory formalism and studying its renormalization as a quantum field theory.
3.2 From Spinfoam Amplitudes to Non-Commutative Field Theory
Besides looking at the quantum gravity corrections to the gravitational interaction, an- other way to probe the semi-classical regime of quantum gravity and extract potential...
==endquote==