Generic framework for non-perturbative QCD in light hadrons
Wei-Yang Liu
TL;DR
This work develops a comprehensive, nonperturbative framework for light-hadron QCD based on the instanton liquid model (ILM). It leverages gradient flow to reveal the topological vacuum structure, introduces a grand canonical ILM to account for fluctuations, and derives a density-expansion with emergent $t\'Hooft$ vertices that map QCD operators and hadronic matrix elements onto effective quark interactions. The framework yields a momentum-dependent constituent quark mass $M(k)$, a calculable gluon condensate, and a topological susceptibility $\chi_t$, with form factors and distribution amplitudes calculable at a low scale $\mu \lesssim 1/ρ$. Predictions show good agreement with lattice QCD, illustrating that a small set of parameters $(ρ,n_{I+A},m)$ controls nonperturbative physics of light hadrons. Overall, the ILM provides a principled, scalable bridge between vacuum topology and hadron phenomenology, enabling systematic calculations of VEVs, hadronic matrix elements, and form factors across scales.
Abstract
This paper aims to serve as an introductory resource for disseminating the concept of instanton liquid model to individuals with interests in quantum chromodynamics (QCD) for hadrons. We discuss several topological aspects of the QCD vacuum and briefly review recent progress on this intuitive unifying framework for the lowlying hadron physics rooted in QCD by introducing the vacuum as a liquid of pseudoparticles. We develop systematic density expansion on the dilute vacuum with diagrammatical Feynman rules to calculate the vacuum expectation values (VEVs) and generalize the calculations to hadronic matrix element (charges), and hadronic form factors using the instanton liquid model (ILM). The ILM prediction are well-consistent with those of recent lattice QCD calculations. Thereby, the nonperturbative physics can be well-controlled by only a few parameters: instanton size $ρ$ and instanton density $n_{I+A}$, and current quark mass $m$.
