SaxiGUTs and their Predictions
Raymond T. Co, Francesco D'Eramo, Lawrence J. Hall

TL;DR
This paper presents a unified supersymmetric axion model predicting dark matter abundance, proton decay, and cosmological signals, with implications for high-scale inflation and supersymmetry breaking.
Contribution
It introduces a novel class of theories linking axion, saxion, and supersymmetry breaking at a high scale, providing detailed predictions for cosmology and particle physics.
Findings
Axion decay constant $f_a$ around $10^{15}$ GeV.
Predicted axion dark matter abundance consistent with initial misalignment angle.
Correlated predictions for proton decay, dark radiation, and inflationary signals.
Abstract
We introduce a class of unified supersymmetric axion theories with unified and PQ symmetries broken by the same set of fields at a scale GeV. A typical domain wall number of order 30 leads to an axion decay constant of order GeV. Inflation generates a large saxion condensate giving a reheat temperature below the QCD scale for supersymmetry breaking of order TeV. Axion field oscillations commence in the saxion matter-dominated era near the QCD scale, and recent lattice computations of the temperature dependence of the axion mass in this era allow a controlled calculation of the axion dark matter abundance. A successful prediction of this abundance results for an initial axion misalignment angle of order unity, . A highly correlated set of predictions is discussed for , , the supersymmetric Higgs mass parameter…
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