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The Problem of Axion Quality: A Low Energy Effective Action Perspective

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arxiv 2207.01068 v1 pith:CKJGZLJO submitted 2022-07-03 hep-ph

classification hep-ph
keywords axionactionsymmetrybreakingproblembeeninstantonsmass
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Any would-be Peccei-Quinn (PQ) symmetry is vulnerable to various types of explicit breaking. It has long been recognized that these can disrupt the axion solution to the strong CP problem. There have also been suggestions that, under certain circumstances, these can lead to a surprisingly large mass for the axion. Two types of corrections to this computation have been widely considered: higher dimension symmetry breaking operators, in theories where there is a complex field responsible for the spontaneous breaking of the PQ symmetry, and small instantons. Motivated by situations where small instantons dominate the $\theta$ potential of non-abelian gauge theories, we formulate the question of axion quality in terms of constraints on a Wilsonian effective action at scales somewhat above the scale of QCD. In this language, the standard axion mass computation assumes a nearly exact PQ symmetry in this action. The higher dimension operators and/or small instantons represent symmetry breaking terms in the Wilsonian action. This picture permits a uniform treatment of the problem of {\it axion quality}. If one assumes order one CP violation at high energies, then solving the strong CP problem constrains the axion potential terms in this Wilsonian action; in particular, the axion mass must be extremely close to its "standard" value.

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Cited by 3 Pith papers

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

  1. Revisiting wormhole-induced global symmetry breaking

    hep-th 2026-07 conditional novelty 6.5 of 10

    Ensemble averaging over wormhole α-parameters is dominated by the symmetric point α=0 for spontaneously broken U(1) p-form symmetries, so standard PQ models evade the wormhole-induced axion quality problem.

  2. First Constraint on Axion-Photon Coupling $g_{\gamma}$ from Neutron Star Observations

    hep-ph 2025-06 reject novelty 6.0 of 10

    The paper derives a first bound on the dimensionless axion-photon coupling gγ from pulsar polarization data, reporting |gγ|<0.93 at 1σ for axion masses below 10^-11 eV, via a neutron-star-induced axion field.

  3. A Non-Inflationary Axion and ALP Misalignment Mechanism

    hep-ph 2025-07 conditional novelty 5.0 of 10

    A thermally mediated, Planck-suppressed symmetry breaking potential can supply the initial axion misalignment that inflationary cosmology normally provides, allowing late-time coherent oscillations without inflation.

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