Quark Schwinger-Dyson equation in temporal Euclidean space
V. Sauli, Z. Batiz

TL;DR
The paper introduces a nonperturbative method to compute Green's functions for timelike momenta in QCD by performing a 3D Wick rotation, revealing complex quark masses and supporting confinement.
Contribution
It presents a novel 3D Wick rotation technique to obtain Green's functions in timelike Euclidean space, applicable to QCD quark propagators, highlighting spontaneous complex mass generation.
Findings
Complex quark mass and wave function generated below perturbative threshold
Method supports confinement via absence of real poles
Equivalent to perturbation theory at weak coupling
Abstract
We present an elementary nonperturbative method to obtain Green's functions (GFs) for timelike momenta. We assume there are no singularities in the first and third quadrants of the complex plane of space momentum components and perform a 3d analogue of Wick rotation. This procedure defines Greens functions in a timelike Euclidean space. As an example we consider the quark propagator in QCD. While for weak coupling, this method is obviously equivalent to perturbation theory, for a realistic QCD coupling a complex part of the quark mass and renormalization wave function has been spontaneously generated even below the standard perturbative threshold. Therefore, our method favors a confinement mechanism based on the lack of real poles.
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Taxonomy
TopicsQuantum Chromodynamics and Particle Interactions · Computational Physics and Python Applications · Particle physics theoretical and experimental studies
