Abstract

Pseudoscalars appear frequently in particle spectra. They can be light if they appear as pseudo-Goldstone bosons from some spontaneously broken global symmetries with the decay constant f. Since any global symmetry is broken at least by quantum gravitational effects, all pseudoscalars are massive. The mass scale of a pseudoscalar is determined by the spontaneous symmetry breaking scale f of the corresponding global symmetry and the explicit breaking terms in the effective potential. The explicit breaking terms can arise from anomaly terms with some non-Abelian gauge groups among which the best-known example is the potential of the QCD axion. Even if there is no breaking terms from gauge anomalies, there can be explicit breaking terms in the potential in which case the leading term suppressed by f determines the pseudoscalar mass scale. If the breaking term is extremely small and the decay constant is trans-Planckian, the corresponding pseudoscalar can be a candidate for a quintessential axion. In the other extreme that the breaking scales are large, still the pseudo-Goldstone boson mass scales are in general smaller than the decay constants. In such a case, still the potential of the pseudo-Goldstone boson at the grand unification scale is sufficiently flat near the top of the potential that it can be a good candidate for an inflationary model. We review these ideas in the bosonic collective motion framework.

Highlights

  • Energy of the Universe is dominated by invisibles: dark energy (DE) composing 68% and dark matter (DM) composing 27% [1]

  • The PQ global symmetry was introduced as a prototype model, which can solve the strong CP problem

  • Pseudoscalars can be made light if they appear as pseudo-Goldstone bosons with the decay constant f

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Summary

Introduction

Energy of the Universe is dominated by invisibles: dark energy (DE) composing 68% and dark matter (DM) composing 27% [1]. DE is about 68% of the critical energy density of the Universe Under this circumstance, I present the BCM idea which can be applicable to all the problems mentioned above, CDM by the “invisible” QCD axion [13,14,15,16], DE by a quintessential axion [24,25], and inflation by “natural” inflation [26,27]. This has led to the Higgs boson acting as a portal to the high energy scale [28,29,30], to the axion scale or even to some standard model (SM) singlets in the grand unification (GUT) scale Can these singlets explain both DE, CDM, and even inflation in the evolving Universe? Can these singlets explain both DE, CDM, and even inflation in the evolving Universe? In this short article, we attempt to answer to this question in the affirmative direction

On Global Symmetries
The ’t Hooft Mechanism
Breaking Scales
The “Invisible” Axion
Axion Inhomogeneities in Galaxies and Mini-Clusters
The Domain Wall Problem in “Invisible” Axion Models
Searches of “Invisible” Axions
A BCM as Dark Energy
Inflation and Gravity Waves in the Beginning
Global Symmetries and Non-Abelian Gauge Groups
Findings
Discussion and Conclusions
Full Text
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