English

Tensorial Gross-Neveu models

High Energy Physics - Theory 2018-10-15 v3

Abstract

We define and study various tensorial generalizations of the Gross-Neveu model in two dimensions, that is, models with four-fermion interactions and G3G^3 symmetry, where we take either G=U(N)G=U(N) or G=O(N)G=O(N). Such models can also be viewed as two-dimensional generalizations of the Sachdev-Ye-Kitaev model, or more precisely of its tensorial counterpart introduced by Klebanov and Tarnopolsky, which is in part our motivation for studying them. Using the Schwinger-Dyson equations at large-NN, we discuss the phenomenon of dynamical mass generation and possible combinations of couplings to avoid it. For the case G=U(N)G=U(N), we introduce an intermediate field representation and perform a stability analysis of the vacua. It turns out that the only apparently viable combination of couplings that avoids mass generation corresponds to an unstable vacuum. The stable vacuum breaks U(N)3U(N)^3 invariance, in contradiction with the Coleman-Mermin-Wagner theorem, but this is an artifact of the large-NN expansion, similar to the breaking of continuous chiral symmetry in the chiral Gross-Neveu model.

Keywords

Cite

@article{arxiv.1710.10253,
  title  = {Tensorial Gross-Neveu models},
  author = {Dario Benedetti and Sylvain Carrozza and Razvan Gurau and Alessandro Sfondrini},
  journal= {arXiv preprint arXiv:1710.10253},
  year   = {2018}
}

Comments

45 pages, 9 figures; v2: new discussion of beta function and IR fixed point in d=2-\epsilon (section 3.2 and appendix C), minor corrections, and references added; v3: minor corrections (mainly concerning figures 3 and 4)

R2 v1 2026-06-22T22:27:56.498Z