Naturally quality-safe GeV axion with charm coupling

Abstract

The GeV-scale QCD axion -- where Peccei-Quinn (PQ) symmetry is broken by the QCD condensate at $f_a\sim \mathcal{O}(1)$~GeV -- faces a structural isospin problem: the PQ spurion coupling to light quarks ($u,d,s$) breaks $\mathrm{SU}(2)$ isospin, generating an unacceptable $\sim 15\%$ $\ddot{I}{€}^0$--$\ddot{I}{€}^{\pm }$ mass splitting. We show that coupling the PQ scalar to the charm quark instead eliminates this violation entirely, and lowering $m_{\ddot{I}}•\sim 3$--$4$~MeV makes the charm Yukawa $\hat{I}{º}_c\propto m_{\ddot{I}}•$ perturbative ($\hat{I}{º}_c<1$). The resulting $f_a\sim \text{GeV}\ll M_{\mathrm{Pl}}$ solves the axion quality problem: even the lowest-dimension $d=6$ Planck-suppressed operator gives $m_{\mathrm{PQ}}/m_a\sim 10^{-14}$, without any additional symmetry. The model predicts a distinctive {\it negative} $\hat{I}”N_{\mathrm{eff}}\sim -0.1$ for $m_{\ddot{I}}•\sim 3$~MeV, testable by CMB-S4. The $B\to K\ddot{I}ƒ$ penguin predicts $\mathrm{BR}\sim 2\times 10^{-5}$, consistent with the Belle~II evidence for $B^{+}\to K^{+}\hat{I}½\bar{\hat{I}}½$ at $(2.3\pm 0.7)\times 10^{-5}$~\cite{BelleII:2024knv}. All ten classes of experimental, astrophysical, and cosmological constraints are satisfied in the viable window $m_{\ddot{I}}•\sim 3$--$4$~MeV, with the $B_s$ mixing constraint pending a dedicated lattice calculation.

5+12 pages, 2+2 tables, 1 figure, comments are welcome

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