Axion and Neutrino physics in a $U(1)$-enhanced supersymmetric model
Y. H. Ahn

TL;DR
This paper proposes a $U(1)$-enhanced supersymmetric model linking axion and neutrino physics, addressing flavor, baryogenesis, and astrophysical issues, and predicts specific neutrino oscillation patterns and axion properties.
Contribution
It introduces a novel $U(1)$ symmetry model that unifies axion and neutrino physics, resolving domain-wall problems and connecting astrophysical constraints with particle physics.
Findings
QCD axion decay constant fixed at ~1.3×10^9 GeV
Neutrino oscillations linked to astronomical scales
Predicted CP phase and mixing angle patterns
Abstract
Motivated by the flavored Peccei-Quinn symmetry for unifying the flavor physics and string theory, we construct an explicit model by introducing a symmetry such that the - anomaly-free condition together with the standard model flavor structure demands additional sterile neutrinos as well as no axionic domain-wall problem. Such additional sterile neutrinos play the role of a realization of baryogenesis via a new Affleck-Dine leptogenesis. We provide grounds for that the symmetry could be interpreted as a fundamental symmetry of nature. The model will resolve rather recent, but fast-growing issues in astro-particle physics, including leptonic mixings and CP violation in neutrino oscillation, high-energy neutrinos, QCD axion, and axion cooling of stars. The QCD axion decay constant, through its connection to the astrophysical constraints of stellar…
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