Discrete Renormalization Group for SU(2) Tensorial Group Field Theory
Sylvain Carrozza
TL;DR
This work develops a Wilsonian, perturbative renormalization group for a rank-3 SU(2) tensorial group field theory and introduces a discrete RG using dimensionless couplings guided by power counting. It shows that melonic graphs dominate UV divergences and derives melonic flow equations, revealing two marginal directions corresponding to the $u_{6,1}$ and $u_{6,2}$ couplings and two unstable directions around the Gaussian fixed point. Second-order corrections demonstrate that positive marginal perturbations do not yield asymptotic freedom, while negative perturbations render the Gaussian fixed point UV-attractive, albeit in a regime that may be non-perturbatively delicate. The results clarify the RG structure of TGFTs and point to potential nontrivial UV behavior, Landau-pole scenarios, or nonperturbative fixed points, motivating future investigations via epsilon-expansion and alternative RG methods.
Abstract
This article provides a Wilsonian description of the perturbatively renormalizable Tensorial Group Field Theory introduced in arXiv:1303.6772 [hep-th] (Commun. Math. Phys. 330, 581-637). It is a rank-3 model based on the gauge group SU(2), and as such is expected to be related to Euclidean quantum gravity in three dimensions. By means of a power-counting argument, we introduce a notion of dimensionality of the free parameters defining the action. General flow equations for the dimensionless bare coupling constants can then be derived, in terms of a discretely varying cut-off, and in which all the so-called melonic Feynman diagrams contribute. Linearizing around the Gaussian fixed point allows to recover the splitting between relevant, irrelevant, and marginal coupling constants. Pushing the perturbative expansion to second order for the marginal parameters, we are able to determine their behaviour in the vicinity of the Gaussian fixed point. Along the way, several technical tools are reviewed, including a discussion of combinatorial factors and of the Laplace approximation, which reduces the evaluation of the amplitudes in the UV limit to that of Gaussian integrals.
