Abstract

We present a unified relaxion solution to the five major outstanding issues in particle physics: the hierarchy problem, dark matter, matter-antimatter asymmetry, neutrino masses and the strong CP problem. The only additional field content in our construction with respect to standard relaxion models is an up-type vector-like fermion pair and three right-handed neutrinos charged under the relaxion shift symmetry. The observed dark matter abundance is generated automatically by oscillations of the relaxion field that begin once it is misaligned from its original stopping point after reheating. The matter-antimatter asymmetry arises from spontaneous baryogenesis induced by the CPT violation due to the rolling of the relaxion after reheating. The CPT violation is communicated to the baryons and leptons via an operator, $\partial_\mu \phi J^\mu$, where $J^\mu$ consists of right-handed neutrino currents arising naturally from a simple neutrino mass model. Finally, the strong CP problem is solved via the Nelson-Barr mechanism, i.e. by imposing CP as a symmetry of the Lagrangian that is broken only spontaneously by the relaxion. The CP breaking is such that although an ${\cal O}(1)$ strong CKM phase is generated, the induced strong CP phase is much smaller, i.e., within experimental bounds.

Highlights

  • Particle physics research has been driven to a large extent by the expectation of physics beyond the Standard Model (BSM) at the TeV scale

  • If Higgs mass naturalness is ignored and new physics scales far beyond the TeV scale are allowed, the other issues can be solved by very minimal extensions of the SM [1,2,3,4,5,6]

  • We show in this paper that the relaxion construction has many interesting built-in features that can provide solutions to multiple other BSM puzzles in a way that is completely different from the other examples referred to above

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Summary

INTRODUCTION

Particle physics research has been driven to a large extent by the expectation of physics beyond the Standard Model (BSM) at the TeV scale. While conventional wisdom says this is impossible, the recently proposed cosmological relaxation (or relaxion) models [7] aim to find just such an explanation In these models the rolling of the so-called relaxion field during inflation leads to a scanning of the Higgs mass squared from positive to negative values. In this work the relaxion shift symmetry is identified with a Froggatt-Nielsen symmetry [14], under which three new right-handed (RH) neutrino states (but no SM states) are charged This satisfies the requirement of spontaneous baryogenesis while giving an explanation for the smallness of neutrino masses.

REVIEW AND BASIC SETUP
Getting the operator OSB
Getting baryon asymmetry from OSB
Neutrino masses
Generating the rolling potential
Nelson-Barr solution to the strong CP problem
PARAMETER SPACE
DISCUSSION AND CONCLUSION
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