Abstract

We find an argument related to the existence of a mathbb {Z}_2-symmetry for the renormalization group flow derived from the bare Yang–Mills Lagrangian, and show that the cancellation of the vacuum energy may arise motivated both from the renormalization group flow solutions and the effective Yang–Mills action. In the framework of the effective Savvidy’s action, two Mirror minima are allowed, with exactly equal and hold opposite sign energy densities. At the cosmological level, we explore the stability of the electric and magnetic attractor solutions, both within and beyond the perturbation theory, and find that thanks to these latter the cancellation between the electric and the magnetic vacua components is achieved at macroscopic space and time separations. This implies the disappearance of the conformal anomaly in the classical limit of an effective Yang–Mills theory. In this picture, the tunneling probability from the Mirror vacua to the other vacua is exponentially suppressed in the quantum non-thermal state – similarly to what happens for electroweak instantonic tunneling solutions. Specifically, we show that, in a dynamical Friedmann–Lemaître–Robertson–Walker (FLRW) cosmological background, the Nielsen–Olsen argument – on the instability of uniform chromo-electric and chromo-magnetic Mirror vacua – is subtly violated. The chromo-magnetic and chromo-electric uniform vacua are unstable only at asymptotic times, but at those times the attractor to a zero energy density is already reached. The two vacua can safely decay into one anisotropic vacuum that has zero energy-density inside the Fermi confinement volume scale. We also discover a new surprising pattern of solitonic and anti-solitonic space-like solutions, which are sourced by the Yang–Mills dynamics coupled to the Einstein’s equations in FLRW. We dub such non-perturbative configurations, which are directly related to dynamical cancellation mechanism of the vacuum energy, as chronons, or chi -solutions.

Highlights

  • The ground state of quantum Yang–Mills (YM) theories plays a crucial role in both particle physics and cosmology

  • From the Quantum Field Theory (QFT) viewpoint, the ground state energy density of the Universe should account for a bulk of various contributions from existing quantum fields, at energy scales ranging from the Quantum Gravity (Planck) scale, MPL 1.2 · 1019 GeV, down to the quantum chromo dynamics (QCD) confinement scale, QCD 0.1 GeV

  • We found an argument for the cancellation of the vacuum energy of QCD in the infrared limit that is related to the existence of an emergent Z2 Mirror symmetry of the RG flow – derived from the bare Lagrangian

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Summary

Introduction

The ground state of quantum Yang–Mills (YM) theories plays a crucial role in both particle physics and cosmology. Even the relatively well-known vacuum subsystems of the Standard Model (SM), such as the Higgs and the quark-gluon condensates, exceed by far the observed CC This is often considered as a severe problem [4,5] – for a recent review on this. QCD, with SU(3) color gauge symmetry, there is a rather unique contribution to the ground state energy of the Universe that emerges from the non-perturbative quantum-topological fluctuations of the quark and gluon fields [1,7,8,9], namely, QCD top. Within this paper we show that even in the framework of standard QFT it is possible to recover as a result the cancellation of SU(2) Yang–Mills (YM) contributions to the vacuum energy within the same theory This achievement holds a certain generality, since SU(2) subgroups of SU(N) YM theories can always be picked out, being the ones that must be accounted for the cosmological applications. Robertson–Walker (FLRW) Universe filled with the gluon condensate, which fluctuates near the minimum of the effective Lagrangian

Effective YM theory and the mirror symmetry
Mirror symmetry
Homogeneous YM condensates
Conclusions and remarks
Effective YM Lagrangian beyond one loop
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