S.M.A.S.H.E.D.: Standard Model Axion Seesaw Higgs Inflation Extended for Dirac Neutrinos
Maximilian Berbig

TL;DR
This paper presents a comprehensive model addressing the strong CP problem, axion dark matter, inflation, and Dirac neutrino masses, with testable predictions for axion experiments and implications for baryogenesis.
Contribution
It introduces a novel extension of the S.M.A.S.H. framework that incorporates Dirac neutrinos, predicts enhanced axion-photon coupling, and demonstrates viable baryogenesis via Dirac-Leptogenesis.
Findings
Predicts an axion-photon coupling larger than conventional models.
Can generate the observed baryon asymmetry through Dirac-Leptogenesis.
Compatible with current bounds on $\, ext{N}_ ext{eff}$.
Abstract
Inspired by the S.M.A.S.H. framework we construct a model that addresses the strong CP problem, axion dark matter, inflation and Dirac neutrino masses as well as leptogenesis. The model possesses only two dynamical scales, namely the SM breaking scale and the Peccei Quinn (PQ) breaking scale . We introduce heavy vector-like quarks in the usual KSVZ fashion to implement the PQ mechanism for the strong CP problem. To generate neutrino masses via a dimension six operator scaling as we add heavy triplet and doublet leptons, which are vector-like under the SM but chiral under PQ symmetry. The model is free from the cosmological domain wall problem and predicts an axion to photon coupling which is about an order of magnitude larger than in conventional DFSZ and KSVZ models. Thus our scenario can be probed and potentially excluded by current and…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories
