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How Viable Is a QCD Axion near 10 MeV?

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arxiv 2405.13425 v2 pith:MJO4BQFL submitted 2024-05-22 hep-ph astro-ph.COhep-exhep-th

How Viable Is a QCD Axion near 10 MeV?

classification hep-ph astro-ph.COhep-exhep-th
keywords modelaxioncontributionelectronmassthereviableanalysis
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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There has been an attempt to revive the visible QCD axion at the 10 MeV scale assuming that it exclusively couples to the first-generation quarks and the electron. This variant of the QCD axion is claimed to remain phenomenologically viable, partly due to a clever model construction that induces tree-level pion-phobia and exploits uncertainties inherent in the chiral perturbation theory. We confront this model with the cosmological domain wall problem, the quality issue and constraints arising from the electron electric dipole moment. It is also pointed out that the gluon loop-generated axion-top coupling can provide a very large contribution to rare $B$-meson decays, such that the present LHCb data for $B^0 \to K^{*0} e^+ e^-$ rule out the model for the axion mass larger than 30 MeV. There is a strong motivation for pushing the experimental analysis of $B \to K^{(*)} e^+ e^-$ to a lower $e^+ e^-$ invariant mass window, which will conclusively determine the fate of the model, as its contribution to this branching ratio significantly exceeds the Standard Model prediction.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Deconstructing the Extra-Dimensional Axion

    hep-ph 2026-06 unverdicted novelty 7.0

    A 4D moose gauge theory with gauged WZW term deconstructs the 5D orbifold axion, reproducing its shift symmetry, instanton effects, and quality features via collective PNGB dynamics.

  2. Looking for Lights from the Darkness: Signals from MeV-scale Solar Axion-like Particles

    hep-ph 2026-04 unverdicted novelty 4.0

    Solar axion-like particles up to 5.5 MeV produce off-axis MeV photons via two-body decay, enabling new space and terrestrial searches that could probe g_aγ down to 10^{-12} GeV^{-1}.