Hybrid SO(10) Axion Model without Quality Problem

Invisible axion models that solve the strong CP problem via the Peccei-Quinn (PQ) mechanism typically have a quality problem that arises from quantum gravity effects which violate all global symmetries. These models therefore require extreme fine-tuning of parameters for consistency. We present a new solution to the quality problem in a unified SO(10)×U(1)_{a} gauge model, where U(1)_{a} is an anomaly free axial gauge symmetry. PQ symmetry emerges as an accidental symmetry in this setup, which admits a PQ breaking scale as large as 7×10^{11} GeV, allowing for the axion to be the cosmological dark matter. We call this a hybrid axion model due to its unique feature that it interpolates between the popular KSVZ and DFSZ axion models. Its predictions for the experimentally measurable axion couplings to the nucleon and electron are distinct from those of the usual models, a feature that can be used to test it. Furthermore, the model has no domain wall problem and it provides a realistic and predictive framework for fermion masses and mixings.

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Publication Details

Journal
Physical Review Letters
Published
2025-03-20
DOI
https://doi.org/10.1103/physrevlett.134.111803
Citations
3
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
5.61

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article

Hybrid SO(10) Axion Model without Quality Problem

Rabindra N. Mohapatra, K. S. Babu, Bhaskar Dutta
3 citations
Physical Review Letters
Dark Matter and Cosmic Phenomena
5.61
article

Hybrid SO(10) Axion Model without Quality Problem

Rabindra N. Mohapatra, K. S. Babu, Bhaskar Dutta
article en
3 citations

Abstract

Invisible axion models that solve the strong CP problem via the Peccei-Quinn (PQ) mechanism typically have a quality problem that arises from quantum gravity effects which violate all global symmetries. These models therefore require extreme fine-tuning of parameters for consistency. We present a new solution to the quality problem in a unified SO(10)×U(1)_{a} gauge model, where U(1)_{a} is an anomaly free axial gauge symmetry. PQ symmetry emerges as an accidental symmetry in this setup, which admits a PQ breaking scale as large as 7×10^{11} GeV, allowing for the axion to be the cosmological dark matter. We call this a hybrid axion model due to its unique feature that it interpolates between the popular KSVZ and DFSZ axion models. Its predictions for the experimentally measurable axion couplings to the nucleon and electron are distinct from those of the usual models, a feature that can be used to test it. Furthermore, the model has no domain wall problem and it provides a realistic and predictive framework for fermion masses and mixings.

Physical Review LettersVol. 134(11)
Mitchell Institute (US), Oklahoma State University Oklahoma City (US), University of Maryland, College Park (US), Texas A&M University (US)
U.S. Department of Energy
Openalex Percentile: Top 6%
Dark Matter and Cosmic Phenomena
5.61
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