English

Gradient properties of $\varphi^3$ in $d=6-\varepsilon$

High Energy Physics - Theory 2025-08-04 v3

Abstract

The renormalization group flow of the multiscalar interacting φ3\varphi^3 theory in d=6d=6 dimensions is known to have a gradient structure, in which suitable generalizations of the beta functions BIB^{I} emerge as the gradient of a scalar function AA, IA=TIJBJ\partial_I A = T_{IJ} B^J , with a nontrivial tensor TIJT_{IJ} in the space of couplings. This has been shown directly to three loops in schemes such as MS\overline{\rm MS} and can be argued in general by identifying AA with the coefficient of the topological term of the trace-anomaly in d=6d=6 up to a normalization. In this paper we show that the same renormalization group has a gradient structure in d=6εd=6-\varepsilon. The requirement of a gradient structure is translated to linear constraints that the coefficients of the MS\overline{\rm MS} beta functions must obey, one of which is new and pertinent only to the extension to d6d \neq 6.

Keywords

Cite

@article{arxiv.2507.20761,
  title  = {Gradient properties of $\varphi^3$ in $d=6-\varepsilon$},
  author = {Lorenzo Benfatto and Omar Zanusso},
  journal= {arXiv preprint arXiv:2507.20761},
  year   = {2025}
}

Comments

8 pages, v2 & v3: improvements and corrections after feedback

R2 v1 2026-07-01T04:21:59.166Z