Abstract:Using a technique devised by Bender, Milton and Savage, we derive the Dyson–Schwinger equations for quantum chromodynamics in differential form. We stop our analysis to the two-point functions. The ’t Hooft limit of color number going to infinity is derived showing how these equations can be cast into a treatable even if approximate form. It is seen how this limit gives a sound description of the low-energy behavior of quantum chromodynamics by discussing the dynamical breaking of chiral symmetry and confineme… Show more
“…where we used the result given in [26] for the non-local Dirac equation and omitted internal degrees of freedom. Anyway, this kind of model can imply breaking of chiral symmetry and confinement as recently shown [64]. This kind of model can also describe bounded states and all the properties of QCD at very low-energy can be translated to the non-local case.…”
Section: Non-local Qcd-like Modelmentioning
confidence: 80%
“…The technique is the following [64]. Let us introduce a set of symbols: η−symbols for SU(N) (this can be possibly extend to the SO(N) case in a straightforward way.…”
“…For the sake of simplicity, we work out the case for SU (2) where the proof of their existence is straightforward. Indeed, in this case, they can be defined as [64,65] η a µ = ((0, 1, 0, 0), (0, 0, 1, 0), (0, 0, 0, 1)),…”
We investigate the non-perturbative regimes in the class of non-Abelian theories that have been proposed as an ultraviolet completion of 4-D Quantum Field Theory (QFT) generalizing the kinetic energy operators to an infinite series of higher-order derivatives inspired by string field theory. We prove that, at the non-perturbative level, the physical spectrum of the theory is actually corrected by the “infinite number of derivatives” present in the action. We derive a set of Dyson-Schwinger equations in differential form, for correlation functions till two-points, the solution for which are known in the local theory. We obtain that just like in the local theory, the non-local counterpart displays a mass gap, depending also on the mass scale of non-locality, and show that it is damped in the deep UV asymptotically. We point out some possible implications of our result in particle physics and cosmology and discuss aspects of non-local QCD-like scenarios.
“…where we used the result given in [26] for the non-local Dirac equation and omitted internal degrees of freedom. Anyway, this kind of model can imply breaking of chiral symmetry and confinement as recently shown [64]. This kind of model can also describe bounded states and all the properties of QCD at very low-energy can be translated to the non-local case.…”
Section: Non-local Qcd-like Modelmentioning
confidence: 80%
“…The technique is the following [64]. Let us introduce a set of symbols: η−symbols for SU(N) (this can be possibly extend to the SO(N) case in a straightforward way.…”
“…For the sake of simplicity, we work out the case for SU (2) where the proof of their existence is straightforward. Indeed, in this case, they can be defined as [64,65] η a µ = ((0, 1, 0, 0), (0, 0, 1, 0), (0, 0, 0, 1)),…”
We investigate the non-perturbative regimes in the class of non-Abelian theories that have been proposed as an ultraviolet completion of 4-D Quantum Field Theory (QFT) generalizing the kinetic energy operators to an infinite series of higher-order derivatives inspired by string field theory. We prove that, at the non-perturbative level, the physical spectrum of the theory is actually corrected by the “infinite number of derivatives” present in the action. We derive a set of Dyson-Schwinger equations in differential form, for correlation functions till two-points, the solution for which are known in the local theory. We obtain that just like in the local theory, the non-local counterpart displays a mass gap, depending also on the mass scale of non-locality, and show that it is damped in the deep UV asymptotically. We point out some possible implications of our result in particle physics and cosmology and discuss aspects of non-local QCD-like scenarios.
“…In order to study these equations, we use the method proposed by Bender, Milton and Savage [13], details of which can found in Refs. [12,[14][15][16][17]. For the purpose of this publication we sketch the main steps here, skipping contributions from BRST ghosts for simplicity.…”
Section: Basic Equations For Njl Modelmentioning
confidence: 99%
“…A first attempt in this direction was given in Ref. [12] in order to determine the proper low-energy limit of the theory 1 . In this work, we fix an error in this publication and show how the effective NJL model comes out naturally from QCD.…”
We evaluate the hadronic contribution to the g − 2 of the muon by deriving the low-energy limit of quantum chromodynamics (QCD) and computing in this way the hadronic vacuum polarization.The low-energy limit is a non-local Nambu-Jona-Lasinio (NJL) model that has all the parameters fixed from QCD, and the only experimental input used is the confinement scale that is known from measurements of hadronic physics. Our estimations provide a novel analytical alternative to the current lattice computations and we find that our result is close to the similar computation performed from experimental data. We also comment on how this analytical approach technique, in general, may provide prospective estimates for hadronic computations from dark sectors and its implication in BSM model-building in future.
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